def generateThumbnails(dir_path, config, mosaic_type, file_list=None):
""" Generates a mosaic of thumbnails from all FF files in the given folder and saves it as a JPG image.
Arguments:
dir_path: [str] Path of the night directory.
config: [Conf object] Configuration.
mosaic_type: [str] Type of the mosaic (e.g. "Captured" or "Detected")
Keyword arguments:
file_list: [list] A list of file names (without full path) which will be searched for FF files. This
is used when generating separate thumbnails for captured and detected files.
Return:
file_name: [str] Name of the thumbnail file.
"""
if file_list is None:
file_list = sorted(os.listdir(dir_path))
# Make a list of all FF files in the night directory
ff_list = []
for file_name in file_list:
if FFfile.validFFName(file_name):
ff_list.append(file_name)
# Calculate the dimensions of the binned image
bin_w = int(config.width/config.thumb_bin)
bin_h = int(config.height/config.thumb_bin)
### RESIZE AND STACK THUMBNAILS ###
##########################################################################################################
timestamps = []
stacked_imgs = []
for i in range(0, len(ff_list), config.thumb_stack):
img_stack = np.zeros((bin_h, bin_w))
# Stack thumb_stack images using the 'if lighter' method
for j in range(config.thumb_stack):
if (i + j) < len(ff_list):
# Read maxpixel image
img = FFfile.read(dir_path, ff_list[i + j]).maxpixel
# Resize the image
img = cv2.resize(img, (bin_w, bin_h))
# Stack the image
img_stack = stackIfLighter(img_stack, img)
else:
break
# Save the timestamp of the first image in the stack
timestamps.append(FFfile.filenameToDatetime(ff_list[i]))
# Save the stacked image
stacked_imgs.append(img_stack)
# cv2.imshow('test', img_stack)
# cv2.waitKey(0)
# cv2.destroyAllWindows()
##########################################################################################################
### ADD THUMBS TO ONE MOSAIC IMAGE ###
##########################################################################################################
header_height = 20
timestamp_height = 10
# Calculate the number of rows for the thumbnail image
n_rows = int(np.ceil(float(len(ff_list))/config.thumb_stack/config.thumb_n_width))
# Calculate the size of the mosaic
mosaic_w = int(config.thumb_n_width*bin_w)
mosaic_h = int((bin_h + timestamp_height)*n_rows + header_height)
mosaic_img = np.zeros((mosaic_h, mosaic_w), dtype=np.uint8)
# Write header text
header_text = 'Station: ' + str(config.stationID) + ' Night: ' + os.path.basename(dir_path) \
+ ' Type: ' + mosaic_type
cv2.putText(mosaic_img, header_text, (0, header_height//2), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255,255,255), 1)
for row in range(n_rows):
for col in range(config.thumb_n_width):
# Calculate image index
indx = row*config.thumb_n_width + col
if indx < len(stacked_imgs):
# Calculate position of the text
text_x = col*bin_w
text_y = row*bin_h + (row + 1)*timestamp_height - 1 + header_height
# Add timestamp text
cv2.putText(mosaic_img, timestamps[indx].strftime('%H:%M:%S'), (text_x, text_y), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255, 255, 255), 1)
# Add the image to the mosaic
img_pos_x = col*bin_w
img_pos_y = row*bin_h + (row + 1)*timestamp_height + header_height
mosaic_img[img_pos_y : img_pos_y + bin_h, img_pos_x : img_pos_x + bin_w] = stacked_imgs[indx]
else:
break
##########################################################################################################
thumb_name = "{:s}_{:s}_{:s}_thumbs.jpg".format(str(config.stationID), os.path.basename(dir_path), \
mosaic_type)
# Save the mosaic
cv2.imwrite(os.path.join(dir_path, thumb_name), mosaic_img, [int(cv2.IMWRITE_JPEG_QUALITY), 80])
return thumb_name
def recalibrateIndividualFFsAndApplyAstrometry(dir_path, ftpdetectinfo_path, calstars_list, config, platepar,
generate_plot=True):
""" Recalibrate FF files with detections and apply the recalibrated platepar to those detections.
Arguments:
dir_path: [str] Path where the FTPdetectinfo file is.
ftpdetectinfo_path: [str] Name of the FTPdetectinfo file.
calstars_list: [list] A list of entries [[ff_name, star_coordinates], ...].
config: [Config instance]
platepar: [Platepar instance] Initial platepar.
Keyword arguments:
generate_plot: [bool] Generate the calibration variation plot. True by default.
Return:
recalibrated_platepars: [dict] A dictionary where the keys are FF file names and values are
recalibrated platepar instances for every FF file.
"""
# Use a copy of the config file
config = copy.deepcopy(config)
# If the given file does not exits, return nothing
if not os.path.isfile(ftpdetectinfo_path):
print('ERROR! The FTPdetectinfo file does not exist: {:s}'.format(ftpdetectinfo_path))
print(' The recalibration on every file was not done!')
return {}
# Read the FTPdetectinfo data
cam_code, fps, meteor_list = FTPdetectinfo.readFTPdetectinfo(*os.path.split(ftpdetectinfo_path), \
ret_input_format=True)
# Convert the list of stars to a per FF name dictionary
calstars = {ff_file: star_data for ff_file, star_data in calstars_list}
### Add neighboring FF files for more robust photometry estimation ###
ff_processing_list = []
# Make a list of sorted FF files in CALSTARS
calstars_ffs = sorted([ff_file for ff_file in calstars])
# Go through the list of FF files with detections and add neighboring FFs
for meteor_entry in meteor_list:
ff_name = meteor_entry[0]
if ff_name in calstars_ffs:
# Find the index of the given FF file in the list of calstars
ff_indx = calstars_ffs.index(ff_name)
# Add neighbours to the processing list
for k in range(-(RECALIBRATE_NEIGHBOURHOOD_SIZE//2), RECALIBRATE_NEIGHBOURHOOD_SIZE//2 + 1):
k_indx = ff_indx + k
if (k_indx > 0) and (k_indx < len(calstars_ffs)):
ff_name_tmp = calstars_ffs[k_indx]
if ff_name_tmp not in ff_processing_list:
ff_processing_list.append(ff_name_tmp)
# Sort the processing list of FF files
ff_processing_list = sorted(ff_processing_list)
### ###
# Globally increase catalog limiting magnitude
config.catalog_mag_limit += 1
# Load catalog stars (overwrite the mag band ratios if specific catalog is used)
star_catalog_status = StarCatalog.readStarCatalog(config.star_catalog_path,\
config.star_catalog_file, lim_mag=config.catalog_mag_limit, \
mag_band_ratios=config.star_catalog_band_ratios)
if not star_catalog_status:
print("Could not load the star catalog!")
print(os.path.join(config.star_catalog_path, config.star_catalog_file))
return {}
catalog_stars, _, config.star_catalog_band_ratios = star_catalog_status
# Update the platepar coordinates from the config file
platepar.lat = config.latitude
platepar.lon = config.longitude
platepar.elev = config.elevation
prev_platepar = copy.deepcopy(platepar)
# Go through all FF files with detections, recalibrate and apply astrometry
recalibrated_platepars = {}
for ff_name in ff_processing_list:
working_platepar = copy.deepcopy(prev_platepar)
# Skip this meteor if its FF file was already recalibrated
if ff_name in recalibrated_platepars:
continue
print()
print('Processing: ', ff_name)
print('------------------------------------------------------------------------------')
# Find extracted stars on this image
if not ff_name in calstars:
print('Skipped because it was not in CALSTARS:', ff_name)
continue
# Get stars detected on this FF file (create a dictionaly with only one entry, the residuals function
# needs this format)
calstars_time = FFfile.getMiddleTimeFF(ff_name, config.fps, ret_milliseconds=True)
jd = date2JD(*calstars_time)
star_dict_ff = {jd: calstars[ff_name]}
# Recalibrate the platepar using star matching
result, min_match_radius = recalibrateFF(config, working_platepar, jd, star_dict_ff, catalog_stars)
# If the recalibration failed, try using FFT alignment
if result is None:
print()
print('Running FFT alignment...')
# Run FFT alignment
calstars_coords = np.array(star_dict_ff[jd])[:, :2]
calstars_coords[:, [0, 1]] = calstars_coords[:, [1, 0]]
print(calstars_time)
test_platepar = alignPlatepar(config, prev_platepar, calstars_time, calstars_coords, \
show_plot=False)
# Try to recalibrate after FFT alignment
result, _ = recalibrateFF(config, test_platepar, jd, star_dict_ff, catalog_stars)
# If the FFT alignment failed, align the original platepar using the smallest radius that matched
# and force save the the platepar
if (result is None) and (min_match_radius is not None):
print()
print("Using the old platepar with the minimum match radius of: {:.2f}".format(min_match_radius))
result, _ = recalibrateFF(config, working_platepar, jd, star_dict_ff, catalog_stars,
max_match_radius=min_match_radius, force_platepar_save=True)
if result is not None:
working_platepar = result
# If the alignment succeeded, save the result
else:
working_platepar = result
else:
working_platepar = result
# Store the platepar if the fit succeeded
if result is not None:
# Recompute alt/az of the FOV centre
working_platepar.az_centre, working_platepar.alt_centre = raDec2AltAz(working_platepar.RA_d, \
working_platepar.dec_d, working_platepar.JD, working_platepar.lat, working_platepar.lon)
# Recompute the rotation wrt horizon
working_platepar.rotation_from_horiz = rotationWrtHorizon(working_platepar)
# Mark the platepar to indicate that it was automatically recalibrated on an individual FF file
working_platepar.auto_recalibrated = True
recalibrated_platepars[ff_name] = working_platepar
prev_platepar = working_platepar
else:
print('Recalibration of {:s} failed, using the previous platepar...'.format(ff_name))
# Mark the platepar to indicate that autorecalib failed
prev_platepar_tmp = copy.deepcopy(prev_platepar)
prev_platepar_tmp.auto_recalibrated = False
# If the aligning failed, set the previous platepar as the one that should be used for this FF file
recalibrated_platepars[ff_name] = prev_platepar_tmp
### Average out photometric offsets within the given neighbourhood size ###
# Go through the list of FF files with detections
for meteor_entry in meteor_list:
ff_name = meteor_entry[0]
# Make sure the FF was successfuly recalibrated
if ff_name in recalibrated_platepars:
# Find the index of the given FF file in the list of calstars
ff_indx = calstars_ffs.index(ff_name)
# Compute the average photometric offset and the improved standard deviation using all
# neighbors
photom_offset_tmp_list = []
photom_offset_std_tmp_list = []
neighboring_ffs = []
for k in range(-(RECALIBRATE_NEIGHBOURHOOD_SIZE//2), RECALIBRATE_NEIGHBOURHOOD_SIZE//2 + 1):
k_indx = ff_indx + k
if (k_indx > 0) and (k_indx < len(calstars_ffs)):
# Get the name of the FF file
ff_name_tmp = calstars_ffs[k_indx]
# Check that the neighboring FF was successfuly recalibrated
if ff_name_tmp in recalibrated_platepars:
# Get the computed photometric offset and stddev
photom_offset_tmp_list.append(recalibrated_platepars[ff_name_tmp].mag_lev)
photom_offset_std_tmp_list.append(recalibrated_platepars[ff_name_tmp].mag_lev_stddev)
neighboring_ffs.append(ff_name_tmp)
# Compute the new photometric offset and improved standard deviation (assume equal sample size)
# Source: https://stats.stackexchange.com/questions/55999/is-it-possible-to-find-the-combined-standard-deviation
photom_offset_new = np.mean(photom_offset_tmp_list)
photom_offset_std_new = np.sqrt(\
np.sum([st**2 + (mt - photom_offset_new)**2 \
for mt, st in zip(photom_offset_tmp_list, photom_offset_std_tmp_list)]) \
/ len(photom_offset_tmp_list)
)
# Assign the new photometric offset and standard deviation to all FFs used for computation
for ff_name_tmp in neighboring_ffs:
recalibrated_platepars[ff_name_tmp].mag_lev = photom_offset_new
recalibrated_platepars[ff_name_tmp].mag_lev_stddev = photom_offset_std_new
### ###
### Store all recalibrated platepars as a JSON file ###
all_pps = {}
for ff_name in recalibrated_platepars:
json_str = recalibrated_platepars[ff_name].jsonStr()
all_pps[ff_name] = json.loads(json_str)
with open(os.path.join(dir_path, config.platepars_recalibrated_name), 'w') as f:
# Convert all platepars to a JSON file
out_str = json.dumps(all_pps, default=lambda o: o.__dict__, indent=4, sort_keys=True)
f.write(out_str)
### ###
# If no platepars were recalibrated, use the single platepar recalibration procedure
if len(recalibrated_platepars) == 0:
print('No FF images were used for recalibration, using the single platepar calibration function...')
# Use the initial platepar for calibration
applyAstrometryFTPdetectinfo(dir_path, os.path.basename(ftpdetectinfo_path), None, platepar=platepar)
return recalibrated_platepars
### GENERATE PLOTS ###
dt_list = []
ang_dists = []
rot_angles = []
hour_list = []
photom_offset_list = []
photom_offset_std_list = []
first_dt = np.min([FFfile.filenameToDatetime(ff_name) for ff_name in recalibrated_platepars])
for ff_name in recalibrated_platepars:
pp_temp = recalibrated_platepars[ff_name]
# If the fitting failed, skip the platepar
if pp_temp is None:
continue
# Add the datetime of the FF file to the list
ff_dt = FFfile.filenameToDatetime(ff_name)
dt_list.append(ff_dt)
# Compute the angular separation from the reference platepar
ang_dist = np.degrees(angularSeparation(np.radians(platepar.RA_d), np.radians(platepar.dec_d), \
np.radians(pp_temp.RA_d), np.radians(pp_temp.dec_d)))
ang_dists.append(ang_dist*60)
# Compute rotation difference
rot_diff = (platepar.pos_angle_ref - pp_temp.pos_angle_ref + 180)%360 - 180
rot_angles.append(rot_diff*60)
# Compute the hour of the FF used for recalibration
hour_list.append((ff_dt - first_dt).total_seconds()/3600)
# Add the photometric offset to the list
photom_offset_list.append(pp_temp.mag_lev)
photom_offset_std_list.append(pp_temp.mag_lev_stddev)
if generate_plot:
# Generate the name the plots
plot_name = os.path.basename(ftpdetectinfo_path).replace('FTPdetectinfo_', '').replace('.txt', '')
### Plot difference from reference platepar in angular distance from (0, 0) vs rotation ###
plt.figure()
plt.scatter(0, 0, marker='o', edgecolor='k', label='Reference platepar', s=100, c='none', zorder=3)
plt.scatter(ang_dists, rot_angles, c=hour_list, zorder=3)
plt.colorbar(label="Hours from first FF file")
plt.xlabel("Angular distance from reference (arcmin)")
plt.ylabel("Rotation from reference (arcmin)")
plt.title("FOV centre drift starting at {:s}".format(first_dt.strftime("%Y/%m/%d %H:%M:%S")))
plt.grid()
plt.legend()
plt.tight_layout()
plt.savefig(os.path.join(dir_path, plot_name + '_calibration_variation.png'), dpi=150)
# plt.show()
plt.clf()
plt.close()
### ###
### Plot the photometric offset variation ###
plt.figure()
plt.errorbar(dt_list, photom_offset_list, yerr=photom_offset_std_list, fmt="o", \
ecolor='lightgray', elinewidth=2, capsize=0, ms=2)
# Format datetimes
plt.gca().xaxis.set_major_formatter(mdates.DateFormatter("%H:%M"))
# rotate and align the tick labels so they look better
plt.gcf().autofmt_xdate()
plt.xlabel("UTC time")
plt.ylabel("Photometric offset")
plt.title("Photometric offset variation")
plt.grid()
plt.tight_layout()
plt.savefig(os.path.join(dir_path, plot_name + '_photometry_variation.png'), dpi=150)
plt.clf()
plt.close()
### ###
### Apply platepars to FTPdetectinfo ###
meteor_output_list = []
for meteor_entry in meteor_list:
ff_name, meteor_No, rho, phi, meteor_meas = meteor_entry
# Get the platepar that will be applied to this FF file
if ff_name in recalibrated_platepars:
working_platepar = recalibrated_platepars[ff_name]
else:
print('Using default platepar for:', ff_name)
working_platepar = platepar
# Apply the recalibrated platepar to meteor centroids
meteor_picks = applyPlateparToCentroids(ff_name, fps, meteor_meas, working_platepar, \
add_calstatus=True)
meteor_output_list.append([ff_name, meteor_No, rho, phi, meteor_picks])
# Calibration string to be written to the FTPdetectinfo file
calib_str = 'Recalibrated with RMS on: ' + str(datetime.datetime.utcnow()) + ' UTC'
# If no meteors were detected, set dummpy parameters
if len(meteor_list) == 0:
cam_code = ''
fps = 0
# Back up the old FTPdetectinfo file
try:
shutil.copy(ftpdetectinfo_path, ftpdetectinfo_path.strip('.txt') \
+ '_backup_{:s}.txt'.format(datetime.datetime.utcnow().strftime('%Y%m%d_%H%M%S.%f')))
except:
print('ERROR! The FTPdetectinfo file could not be backed up: {:s}'.format(ftpdetectinfo_path))
# Save the updated FTPdetectinfo
FTPdetectinfo.writeFTPdetectinfo(meteor_output_list, dir_path, os.path.basename(ftpdetectinfo_path), \
dir_path, cam_code, fps, calibration=calib_str, celestial_coords_given=True)
### ###
return recalibrated_platepars
def generateThumbnails(dir_path,
config,
mosaic_type,
file_list=None,
no_stack=False):
""" Generates a mosaic of thumbnails from all FF files in the given folder and saves it as a JPG image.
Arguments:
dir_path: [str] Path of the night directory.
config: [Conf object] Configuration.
mosaic_type: [str] Type of the mosaic (e.g. "Captured" or "Detected")
Keyword arguments:
file_list: [list] A list of file names (without full path) which will be searched for FF files. This
is used when generating separate thumbnails for captured and detected files.
Return:
file_name: [str] Name of the thumbnail file.
no_stack: [bool] Don't stack the images using the config.thumb_stack option. A max of 1000 images
are supported with this option. If there are more, stacks will be done according to the
config.thumb_stack option.
"""
if file_list is None:
file_list = sorted(os.listdir(dir_path))
# Make a list of all FF files in the night directory
ff_list = []
for file_name in file_list:
if FFfile.validFFName(file_name):
ff_list.append(file_name)
# Calculate the dimensions of the binned image
bin_w = int(config.width / config.thumb_bin)
bin_h = int(config.height / config.thumb_bin)
### RESIZE AND STACK THUMBNAILS ###
##########################################################################################################
timestamps = []
stacked_imgs = []
thumb_stack = config.thumb_stack
# Check if no stacks should be done (max 1000 images for no stack)
if no_stack and (len(ff_list) < 1000):
thumb_stack = 1
for i in range(0, len(ff_list), thumb_stack):
img_stack = np.zeros((bin_h, bin_w))
# Stack thumb_stack images using the 'if lighter' method
for j in range(thumb_stack):
if (i + j) < len(ff_list):
tmp_file_name = ff_list[i + j]
# Read the FF file
ff = FFfile.read(dir_path, tmp_file_name)
# Skip the FF if it is corruped
if ff is None:
continue
img = ff.maxpixel
# Resize the image
img = cv2.resize(img, (bin_w, bin_h))
# Stack the image
img_stack = stackIfLighter(img_stack, img)
else:
break
# Save the timestamp of the first image in the stack
timestamps.append(FFfile.filenameToDatetime(ff_list[i]))
# Save the stacked image
stacked_imgs.append(img_stack)
# cv2.imshow('test', img_stack)
# cv2.waitKey(0)
# cv2.destroyAllWindows()
##########################################################################################################
### ADD THUMBS TO ONE MOSAIC IMAGE ###
##########################################################################################################
header_height = 20
timestamp_height = 10
# Calculate the number of rows for the thumbnail image
n_rows = int(
np.ceil(float(len(ff_list)) / thumb_stack / config.thumb_n_width))
# Calculate the size of the mosaic
mosaic_w = int(config.thumb_n_width * bin_w)
mosaic_h = int((bin_h + timestamp_height) * n_rows + header_height)
mosaic_img = np.zeros((mosaic_h, mosaic_w), dtype=np.uint8)
# Write header text
header_text = 'Station: ' + str(config.stationID) + ' Night: ' + os.path.basename(dir_path) \
+ ' Type: ' + mosaic_type
cv2.putText(mosaic_img, header_text, (0, header_height//2), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255,255,255), 1)
for row in range(n_rows):
for col in range(config.thumb_n_width):
# Calculate image index
indx = row * config.thumb_n_width + col
if indx < len(stacked_imgs):
# Calculate position of the text
text_x = col * bin_w
text_y = row * bin_h + (
row + 1) * timestamp_height - 1 + header_height
# Add timestamp text
cv2.putText(mosaic_img, timestamps[indx].strftime('%H:%M:%S'), (text_x, text_y), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255, 255, 255), 1)
# Add the image to the mosaic
img_pos_x = col * bin_w
img_pos_y = row * bin_h + (
row + 1) * timestamp_height + header_height
mosaic_img[img_pos_y:img_pos_y + bin_h,
img_pos_x:img_pos_x + bin_w] = stacked_imgs[indx]
else:
break
##########################################################################################################
# Only add the station ID if the dir name already doesn't start with it
dir_name = os.path.basename(os.path.abspath(dir_path))
if dir_name.startswith(config.stationID):
prefix = dir_name
else:
prefix = "{:s}_{:s}".format(config.stationID, dir_name)
thumb_name = "{:s}_{:s}_thumbs.jpg".format(prefix, mosaic_type)
# Save the mosaic
if USING_IMAGEIO:
# Use imageio to write the image
imwrite(os.path.join(dir_path, thumb_name), mosaic_img, quality=80)
else:
# Use OpenCV to save the image
imwrite(os.path.join(dir_path, thumb_name), mosaic_img,
[int(cv2.IMWRITE_JPEG_QUALITY), 80])
return thumb_name
def generateThumbnails(dir_path, config, mosaic_type, file_list=None):
""" Generates a mosaic of thumbnails from all FF files in the given folder and saves it as a JPG image.
Arguments:
dir_path: [str] Path of the night directory.
config: [Conf object] Configuration.
mosaic_type: [str] Type of the mosaic (e.g. "Captured" or "Detected")
Keyword arguments:
file_list: [list] A list of file names (without full path) which will be searched for FF files. This
is used when generating separate thumbnails for captured and detected files.
Return:
file_name: [str] Name of the thumbnail file.
"""
if file_list is None:
file_list = sorted(os.listdir(dir_path))
# Make a list of all FF files in the night directory
ff_list = []
for file_name in file_list:
if FFfile.validFFName(file_name):
ff_list.append(file_name)
# Calculate the dimensions of the binned image
bin_w = int(config.width/config.thumb_bin)
bin_h = int(config.height/config.thumb_bin)
### RESIZE AND STACK THUMBNAILS ###
##########################################################################################################
timestamps = []
stacked_imgs = []
for i in range(0, len(ff_list), config.thumb_stack):
img_stack = np.zeros((bin_h, bin_w))
# Stack thumb_stack images using the 'if lighter' method
for j in range(config.thumb_stack):
if (i + j) < len(ff_list):
tmp_file_name = ff_list[i + j]
# Read the FF file
ff = FFfile.read(dir_path, tmp_file_name)
# Skip the FF if it is corruped
if ff is None:
continue
img = ff.maxpixel
# Resize the image
img = cv2.resize(img, (bin_w, bin_h))
# Stack the image
img_stack = stackIfLighter(img_stack, img)
else:
break
# Save the timestamp of the first image in the stack
timestamps.append(FFfile.filenameToDatetime(ff_list[i]))
# Save the stacked image
stacked_imgs.append(img_stack)
# cv2.imshow('test', img_stack)
# cv2.waitKey(0)
# cv2.destroyAllWindows()
##########################################################################################################
### ADD THUMBS TO ONE MOSAIC IMAGE ###
##########################################################################################################
header_height = 20
timestamp_height = 10
# Calculate the number of rows for the thumbnail image
n_rows = int(np.ceil(float(len(ff_list))/config.thumb_stack/config.thumb_n_width))
# Calculate the size of the mosaic
mosaic_w = int(config.thumb_n_width*bin_w)
mosaic_h = int((bin_h + timestamp_height)*n_rows + header_height)
mosaic_img = np.zeros((mosaic_h, mosaic_w), dtype=np.uint8)
# Write header text
header_text = 'Station: ' + str(config.stationID) + ' Night: ' + os.path.basename(dir_path) \
+ ' Type: ' + mosaic_type
cv2.putText(mosaic_img, header_text, (0, header_height//2), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255,255,255), 1)
for row in range(n_rows):
for col in range(config.thumb_n_width):
# Calculate image index
indx = row*config.thumb_n_width + col
if indx < len(stacked_imgs):
# Calculate position of the text
text_x = col*bin_w
text_y = row*bin_h + (row + 1)*timestamp_height - 1 + header_height
# Add timestamp text
cv2.putText(mosaic_img, timestamps[indx].strftime('%H:%M:%S'), (text_x, text_y), \
cv2.FONT_HERSHEY_SIMPLEX, 0.4, (255, 255, 255), 1)
# Add the image to the mosaic
img_pos_x = col*bin_w
img_pos_y = row*bin_h + (row + 1)*timestamp_height + header_height
mosaic_img[img_pos_y : img_pos_y + bin_h, img_pos_x : img_pos_x + bin_w] = stacked_imgs[indx]
else:
break
##########################################################################################################
thumb_name = "{:s}_{:s}_{:s}_thumbs.jpg".format(str(config.stationID), os.path.basename(dir_path), \
mosaic_type)
# Save the mosaic
cv2.imwrite(os.path.join(dir_path, thumb_name), mosaic_img, [int(cv2.IMWRITE_JPEG_QUALITY), 80])
return thumb_name
def FTPdetectinfo2UFOOrbitInput(dir_path, file_name, platepar_path, platepar_dict=None):
""" Convert the FTPdetectinfo file into UFOOrbit input CSV file.
Arguments:
dir_path: [str] Path of the directory which contains the FTPdetectinfo file.
file_name: [str] Name of the FTPdetectinfo file.
platepar_path: [str] Full path to the platepar file.
Keyword arguments:
platepar_dict: [dict] Dictionary of Platepar instances where keys are FF file names. This will be
used instead of the platepar at platepar_path. None by default.
"""
# Load the FTPdetecinfo file
meteor_list = FTPdetectinfo.readFTPdetectinfo(dir_path, file_name)
# Load the platepar file
if platepar_dict is None:
pp = RMS.Formats.Platepar.Platepar()
pp.read(platepar_path)
# Init the UFO format list
ufo_meteor_list = []
# Go through every meteor in the list
for meteor in meteor_list:
ff_name, cam_code, meteor_No, n_segments, fps, hnr, mle, binn, px_fm, rho, phi, \
meteor_meas = meteor
# Load the platepar from the platepar dictionary, if given
if platepar_dict is not None:
if ff_name in platepar_dict:
pp = platepar_dict[ff_name]
else:
print('Skipping {:s} becuase no platepar was found for this FF file!'.format(ff_name))
# Convert the FF file name into time
dt = FFfile.filenameToDatetime(ff_name)
# Extract measurements
calib_status, frame_n, x, y, ra, dec, azim, elev, inten, mag = np.array(meteor_meas).T
# If the meteor wasn't calibrated, skip it
if not np.all(calib_status):
print('Meteor {:d} was not calibrated, skipping it...'.format(meteor_No))
continue
# Compute the peak magnitude
peak_mag = np.min(mag)
# Compute the total duration
first_frame = np.min(frame_n)
last_frame = np.max(frame_n)
duration = (last_frame - first_frame)/fps
# Compute times of first and last points
dt1 = dt + datetime.timedelta(seconds=first_frame/fps)
dt2 = dt + datetime.timedelta(seconds=last_frame/fps)
### Fit a great circle to Az/Alt measurements and compute model beg/end RA and Dec ###
# Convert the measurement Az/Alt to cartesian coordinates
# NOTE: All values that are used for Great Circle computation are:
# theta - the zenith angle (90 deg - altitude)
# phi - azimuth +N of due E, which is (90 deg - azim)
x, y, z = Math.polarToCartesian(np.radians((90 - azim)%360), np.radians(90 - elev))
# Fit a great circle
C, theta0, phi0 = GreatCircle.fitGreatCircle(x, y, z)
# Get the first point on the great circle
phase1 = GreatCircle.greatCirclePhase(np.radians(90 - elev[0]), np.radians((90 - azim[0])%360), \
theta0, phi0)
alt1, azim1 = Math.cartesianToPolar(*GreatCircle.greatCircle(phase1, theta0, phi0))
alt1 = 90 - np.degrees(alt1)
azim1 = (90 - np.degrees(azim1))%360
# Get the last point on the great circle
phase2 = GreatCircle.greatCirclePhase(np.radians(90 - elev[-1]), np.radians((90 - azim[-1])%360),\
theta0, phi0)
alt2, azim2 = Math.cartesianToPolar(*GreatCircle.greatCircle(phase2, theta0, phi0))
alt2 = 90 - np.degrees(alt2)
azim2 = (90 - np.degrees(azim2))%360
# Compute RA/Dec from Alt/Az
_, ra1, dec1 = RMS.Astrometry.ApplyAstrometry.altAzToRADec(pp.lat, pp.lon, pp.UT_corr, [dt1], \
[azim1], [alt1], dt_time=True)
_, ra2, dec2 = RMS.Astrometry.ApplyAstrometry.altAzToRADec(pp.lat, pp.lon, pp.UT_corr, [dt2], \
[azim2], [alt2], dt_time=True)
### ###
ufo_meteor_list.append([dt1, peak_mag, duration, azim1[0], alt1[0], azim2[0], alt2[0], \
ra1[0][0], dec1[0][0], ra2[0][0], dec2[0][0], cam_code, pp.lon, pp.lat, pp.elev, pp.UT_corr])
# Construct a file name for the UFO file, which is the FTPdetectinfo file without the FTPdetectinfo
# part
ufo_file_name = file_name.replace('FTPdetectinfo_', '').replace('.txt', '') + '.csv'
# Write the UFOorbit file
UFOOrbit.writeUFOOrbit(dir_path, ufo_file_name, ufo_meteor_list)
def FTPdetectinfo2UFOOrbitInput(dir_path,
file_name,
platepar_path,
platepar_dict=None):
""" Convert the FTPdetectinfo file into UFOOrbit input CSV file.
Arguments:
dir_path: [str] Path of the directory which contains the FTPdetectinfo file.
file_name: [str] Name of the FTPdetectinfo file.
platepar_path: [str] Full path to the platepar file.
Keyword arguments:
platepar_dict: [dict] Dictionary of Platepar instances where keys are FF file names. This will be
used instead of the platepar at platepar_path. None by default.
"""
# Load the FTPdetecinfo file
meteor_list = FTPdetectinfo.readFTPdetectinfo(dir_path, file_name)
# Load the platepar file
if platepar_dict is None:
pp = RMS.Formats.Platepar.Platepar()
pp.read(platepar_path, use_flat=None)
# Init the UFO format list
ufo_meteor_list = []
# Go through every meteor in the list
for meteor in meteor_list:
ff_name, cam_code, meteor_No, n_segments, fps, hnr, mle, binn, px_fm, rho, phi, \
meteor_meas = meteor
# Load the platepar from the platepar dictionary, if given
if platepar_dict is not None:
if ff_name in platepar_dict:
pp = platepar_dict[ff_name]
else:
print(
'Skipping {:s} becuase no platepar was found for this FF file!'
.format(ff_name))
continue
# Convert the FF file name into time
dt = FFfile.filenameToDatetime(ff_name)
# Extract measurements
calib_status, frame_n, x, y, ra, dec, azim, elev, inten, mag = np.array(
meteor_meas).T
# If the meteor wasn't calibrated, skip it
if not np.all(calib_status):
print('Meteor {:d} was not calibrated, skipping it...'.format(
meteor_No))
continue
# Compute the peak magnitude
peak_mag = np.min(mag)
# Compute the total duration
first_frame = np.min(frame_n)
last_frame = np.max(frame_n)
duration = (last_frame - first_frame) / fps
# Compute times of first and last points
dt1 = dt + datetime.timedelta(seconds=first_frame / fps)
dt2 = dt + datetime.timedelta(seconds=last_frame / fps)
### Fit a great circle to Az/Alt measurements and compute model beg/end RA and Dec ###
# Convert the measurement Az/Alt to cartesian coordinates
# NOTE: All values that are used for Great Circle computation are:
# theta - the zenith angle (90 deg - altitude)
# phi - azimuth +N of due E, which is (90 deg - azim)
x, y, z = Math.polarToCartesian(np.radians((90 - azim) % 360),
np.radians(90 - elev))
# Fit a great circle
C, theta0, phi0 = GreatCircle.fitGreatCircle(x, y, z)
# Get the first point on the great circle
phase1 = GreatCircle.greatCirclePhase(np.radians(90 - elev[0]), np.radians((90 - azim[0])%360), \
theta0, phi0)
alt1, azim1 = Math.cartesianToPolar(
*GreatCircle.greatCircle(phase1, theta0, phi0))
alt1 = 90 - np.degrees(alt1)
azim1 = (90 - np.degrees(azim1)) % 360
# Get the last point on the great circle
phase2 = GreatCircle.greatCirclePhase(np.radians(90 - elev[-1]), np.radians((90 - azim[-1])%360),\
theta0, phi0)
alt2, azim2 = Math.cartesianToPolar(
*GreatCircle.greatCircle(phase2, theta0, phi0))
alt2 = 90 - np.degrees(alt2)
azim2 = (90 - np.degrees(azim2)) % 360
# Compute RA/Dec from Alt/Az
_, ra1, dec1 = RMS.Astrometry.ApplyAstrometry.altAzToRADec(pp.lat, pp.lon, pp.UT_corr, [dt1], \
[azim1], [alt1], dt_time=True)
_, ra2, dec2 = RMS.Astrometry.ApplyAstrometry.altAzToRADec(pp.lat, pp.lon, pp.UT_corr, [dt2], \
[azim2], [alt2], dt_time=True)
### ###
ufo_meteor_list.append([dt1, peak_mag, duration, azim1[0], alt1[0], azim2[0], alt2[0], \
ra1[0][0], dec1[0][0], ra2[0][0], dec2[0][0], cam_code, pp.lon, pp.lat, pp.elev, pp.UT_corr])
# Construct a file name for the UFO file, which is the FTPdetectinfo file without the FTPdetectinfo
# part
ufo_file_name = file_name.replace('FTPdetectinfo_', '').replace(
'.txt', '') + '.csv'
# Write the UFOorbit file
UFOOrbit.writeUFOOrbit(dir_path, ufo_file_name, ufo_meteor_list)
def recalibrateIndividualFFsAndApplyAstrometry(dir_path, ftpdetectinfo_path, calstars_list, config, platepar):
""" Recalibrate FF files with detections and apply the recalibrated platepar to those detections.
Arguments:
dir_path: [str] Path where the FTPdetectinfo file is.
ftpdetectinfo_path: [str] Name of the FTPdetectinfo file.
calstars_list: [list] A list of entries [[ff_name, star_coordinates], ...].
config: [Config instance]
platepar: [Platepar instance] Initial platepar.
Return:
recalibrated_platepars: [dict] A dictionary where the keys are FF file names and values are
recalibrated platepar instances for every FF file.
"""
# Read the FTPdetectinfo data
cam_code, fps, meteor_list = FTPdetectinfo.readFTPdetectinfo(*os.path.split(ftpdetectinfo_path), \
ret_input_format=True)
# Convert the list of stars to a per FF name dictionary
calstars = {ff_file: star_data for ff_file, star_data in calstars_list}
# Load catalog stars (overwrite the mag band ratios if specific catalog is used)
catalog_stars, _, config.star_catalog_band_ratios = StarCatalog.readStarCatalog(config.star_catalog_path,\
config.star_catalog_file, lim_mag=config.catalog_mag_limit, \
mag_band_ratios=config.star_catalog_band_ratios)
prev_platepar = copy.deepcopy(platepar)
# Go through all FF files with detections, recalibrate and apply astrometry
recalibrated_platepars = {}
for meteor_entry in meteor_list:
working_platepar = copy.deepcopy(prev_platepar)
ff_name, meteor_No, rho, phi, meteor_meas = meteor_entry
# Skip this meteors if its FF file was already recalibrated
if ff_name in recalibrated_platepars:
continue
print()
print('Processing: ', ff_name)
print('------------------------------------------------------------------------------')
# Find extracted stars on this image
if not ff_name in calstars:
print('Skipped because it was not in CALSTARS:', ff_name)
continue
# Get stars detected on this FF file (create a dictionaly with only one entry, the residuals function
# needs this format)
calstars_time = FFfile.getMiddleTimeFF(ff_name, config.fps, ret_milliseconds=True)
jd = date2JD(*calstars_time)
star_dict_ff = {jd: calstars[ff_name]}
# Recalibrate the platepar using star matching
result = recalibrateFF(config, working_platepar, jd, star_dict_ff, catalog_stars)
# If the recalibration failed, try using FFT alignment
if result is None:
print()
print('Running FFT alignment...')
# Run FFT alignment
calstars_coords = np.array(star_dict_ff[jd])[:, :2]
calstars_coords[:, [0, 1]] = calstars_coords[:, [1, 0]]
print(calstars_time)
working_platepar = alignPlatepar(config, prev_platepar, calstars_time, calstars_coords, \
show_plot=False)
# Try to recalibrate after FFT alignment
result = recalibrateFF(config, working_platepar, jd, star_dict_ff, catalog_stars)
if result is not None:
working_platepar = result
else:
working_platepar = result
# Store the platepar if the fit succeeded
if result is not None:
recalibrated_platepars[ff_name] = working_platepar
prev_platepar = working_platepar
else:
print('Recalibration of {:s} failed, using the previous platepar...'.format(ff_name))
# If the aligning failed, set the previous platepar as the one that should be used for this FF file
recalibrated_platepars[ff_name] = prev_platepar
### Store all recalibrated platepars as a JSON file ###
all_pps = {}
for ff_name in recalibrated_platepars:
json_str = recalibrated_platepars[ff_name].jsonStr()
all_pps[ff_name] = json.loads(json_str)
with open(os.path.join(dir_path, config.platepars_recalibrated_name), 'w') as f:
# Convert all platepars to a JSON file
out_str = json.dumps(all_pps, default=lambda o: o.__dict__, indent=4, sort_keys=True)
f.write(out_str)
### ###
# If no platepars were recalibrated, use the single platepar recalibration procedure
if len(recalibrated_platepars) == 0:
print('No FF images were used for recalibration, using the single platepar calibration function...')
# Use the initial platepar for calibration
applyAstrometryFTPdetectinfo(dir_path, os.path.basename(ftpdetectinfo_path), None, platepar=platepar)
return recalibrated_platepars
### Plot difference from reference platepar in angular distance from (0, 0) vs rotation ###
ang_dists = []
rot_angles = []
hour_list = []
first_jd = np.min([FFfile.filenameToDatetime(ff_name) for ff_name in recalibrated_platepars])
for ff_name in recalibrated_platepars:
pp_temp = recalibrated_platepars[ff_name]
# If the fitting failed, skip the platepar
if pp_temp is None:
continue
# Compute the angular separation from the reference platepar
ang_dist = np.degrees(angularSeparation(np.radians(platepar.RA_d), np.radians(platepar.dec_d), \
np.radians(pp_temp.RA_d), np.radians(pp_temp.dec_d)))
ang_dists.append(ang_dist*60)
rot_angles.append((platepar.pos_angle_ref - pp_temp.pos_angle_ref)*60)
# Compute the hour of the FF used for recalibration
hour_list.append((FFfile.filenameToDatetime(ff_name) - first_jd).total_seconds()/3600)
plt.figure()
plt.scatter(0, 0, marker='o', edgecolor='k', label='Reference platepar', s=100, c='none', zorder=3)
plt.scatter(ang_dists, rot_angles, c=hour_list, zorder=3)
plt.colorbar(label='Hours from first FF file')
plt.xlabel("Angular distance from reference (arcmin)")
plt.ylabel('Rotation from reference (arcmin)')
plt.grid()
plt.legend()
plt.tight_layout()
# Generate the name for the plot
calib_plot_name = os.path.basename(ftpdetectinfo_path).replace('FTPdetectinfo_', '').replace('.txt', '') \
+ '_calibration_variation.png'
plt.savefig(os.path.join(dir_path, calib_plot_name), dpi=150)
# plt.show()
plt.clf()
plt.close()
### ###
### Apply platepars to FTPdetectinfo ###
meteor_output_list = []
for meteor_entry in meteor_list:
ff_name, meteor_No, rho, phi, meteor_meas = meteor_entry
# Get the platepar that will be applied to this FF file
if ff_name in recalibrated_platepars:
working_platepar = recalibrated_platepars[ff_name]
else:
print('Using default platepar for:', ff_name)
working_platepar = platepar
# Apply the recalibrated platepar to meteor centroids
meteor_picks = applyPlateparToCentroids(ff_name, fps, meteor_meas, working_platepar, \
add_calstatus=True)
meteor_output_list.append([ff_name, meteor_No, rho, phi, meteor_picks])
# Calibration string to be written to the FTPdetectinfo file
calib_str = 'Recalibrated with RMS on: ' + str(datetime.datetime.utcnow()) + ' UTC'
# If no meteors were detected, set dummpy parameters
if len(meteor_list) == 0:
cam_code = ''
fps = 0
# Back up the old FTPdetectinfo file
shutil.copy(ftpdetectinfo_path, ftpdetectinfo_path.strip('.txt') \
+ '_backup_{:s}.txt'.format(datetime.datetime.utcnow().strftime('%Y%m%d_%H%M%S.%f')))
# Save the updated FTPdetectinfo
FTPdetectinfo.writeFTPdetectinfo(meteor_output_list, dir_path, os.path.basename(ftpdetectinfo_path), \
dir_path, cam_code, fps, calibration=calib_str, celestial_coords_given=True)
### ###
return recalibrated_platepars
