示例#1
0
def grid_relh(nc, ts, rs):
    lats = []
    lons = []
    vals = []
    for i in range(len(rs)):
        if rs[i]['max_tmpf'] is not None and rs[i]['max_dwpf'] is not None:
            lats.append(  locs[rs[i]['station']]['lat'] )
            lons.append(  locs[rs[i]['station']]['lon'] )
            vals.append( mesonet.relh( rs[i]['max_tmpf'], rs[i]['max_dwpf'] ) )
    if len(vals) < 4:
        print "No RELH data at all for time: %s" % (ts,)   
        return
    grid = Ngl.natgrid(lons, lats, vals, XAXIS, YAXIS)
    offset = int((ts - BASE).hours )
    if grid is not None:
        gt = grid.transpose()
        gt = numpy.where(gt < 100.1, gt, 100.)
        nc.variables['relh'][offset,:,:] = numpy.where(gt < 12., 12., gt)
    else:
        print "RELH gridding failed, len vals %s" % (len(vals),)
示例#2
0
文件: spaghetti.py 项目: bthoover/iem
    relh = []
    vsby = []
    raining = False
    for row2 in acursor2:
        if row2[3] >= maxD and row2[1] >= 100:
            print row2[0], row2[3]
            maxD = row2[3]
        if row2[2] > 0:
            raining = True
        if len(times) > 10 and row2[0].hour == 0:
            times.append(row2[0].hour * 60 + row2[0].minute + 1440)
        else:
            times.append(row2[0].hour * 60 + row2[0].minute)
        if row2[0].hour in [5, 9]:
            print row2
        relh.append(mesonet.relh(row2[1], row2[3]))
        vsby.append(row2[4])

    # c = '#E8AFAF'
    # if raining:
    #    c = 'b'
    c = colors.pop()
    ax.plot(times, relh, c=c, label=station)
    ax2.plot(times, vsby, linestyle="--", c=c)
# ax.plot( [6*60, 10*60, 10*60, 6*60,6*60], [69,75,84,77,69] , c='black')
# ax.text(6*60, 66, "6-10 AM Diff: %.1f$^{\circ}\mathrm{F}$" % ((diff/3.,) ))
#
# ax.text(14*60, 66, "Newton, IA (KTNU AWOS)")


ax.grid(True)
示例#3
0
文件: ragbrai.py 项目: nbackas/iem
#output = open('ragbrai.dat', 'w')
for sdate, edate in DATES:
    acursor.execute("""
    SELECT tmpf, dwpf, sknt, drct, valid from t%s WHERE station = 'DSM' and valid BETWEEN '%s 00:00' and '%s 23:59' and tmpf > 0
    and dwpf > 0 and sknt >= 0 and drct >= 0 ORDER by valid ASC
    """ % (sdate.year, sdate.strftime("%Y-%m-%d"), edate.strftime("%Y-%m-%d")))
    cnt = 0
    tot = 0
    ttot = 0
    utot = 0
    ucnt = 0
    vtot = 0
    for row in acursor:
        ttot += row[0]
        h = mesonet.heatidx(row[0], mesonet.relh(row[0], row[1]))
        if row[4].hour > 5 and row[4].hour < 22:
            u, v = uv(row[2], row[3])
            #output.write("%s,%s,%s,%.1f,%.2f,%.2f\n" % (row[4].strftime("%Y,%m,%d,%H,%M"), row[0], row[1], h, u, v))
            utot += u
            vtot += v
            ucnt += 1
        tot += h
        cnt += 1
    print "%s %3s %4.1f %4.1f %4.1f %4.1f" % (
        sdate.year, cnt, ttot / float(cnt), tot / float(cnt),
        utot / float(ucnt), vtot / float(ucnt))
    uwnd[sdate.year - 1973] = utot / float(ucnt) * 1.15
    hindex[sdate.year - 1973] = tot / float(cnt)
#output.close()
示例#4
0
文件: ragbrai.py 项目: akrherz/DEV
#output = open('ragbrai.dat', 'w')
for sdate,edate in DATES:
    acursor.execute("""
    SELECT tmpf, dwpf, sknt, drct, valid from t%s WHERE station = 'DSM' and valid BETWEEN '%s 00:00' and '%s 23:59' and tmpf > 0
    and dwpf > 0 and sknt >= 0 and drct >= 0 ORDER by valid ASC
    """ % (sdate.year, sdate.strftime("%Y-%m-%d"), edate.strftime("%Y-%m-%d") ))
    cnt = 0
    tot = 0
    ttot = 0
    utot = 0
    ucnt = 0
    vtot = 0
    for row in acursor:
        ttot += row[0]
        h = mesonet.heatidx(row[0], mesonet.relh(row[0], row[1]))
        if row[4].hour > 5 and row[4].hour < 22:
            u,v = uv(row[2], row[3])
        #output.write("%s,%s,%s,%.1f,%.2f,%.2f\n" % (row[4].strftime("%Y,%m,%d,%H,%M"), row[0], row[1], h, u, v))
            utot += u
            vtot += v
            ucnt += 1
        tot += h
        cnt += 1
    print "%s %3s %4.1f %4.1f %4.1f %4.1f" % (sdate.year, cnt, ttot / float(cnt), tot / float(cnt), utot / float(ucnt), vtot / float(ucnt))
    uwnd[sdate.year-1973] = utot / float(ucnt) * 1.15
    hindex[sdate.year-1973] = tot / float(cnt)
#output.close()

import matplotlib.pyplot as plt
fig = plt.figure()
示例#5
0
文件: asos2hcd.py 项目: akrherz/MSDOT
    sql = "SELECT *, \
   case when sknt > 0 THEN sknt ELSE 0 END as sknt0,\
   case when p01m > 0 THEN p01m ELSE 0 END as p,\
   case when skyc > -1 THEN skyc ELSE 0 END as sk from t%s WHERE station = '%s' and tmpf > -50 and extract(year from valid) = %s ORDER by valid ASC" % (
        yr, stid, yr)
    rs = asos.query(sql).dictresult()
    for i in range(len(rs)):
        ts = mx.DateTime.strptime(rs[i]['valid'][:13], "%Y-%m-%d %H")
        if (now == ts):
            #print 'DUP', now
            continue
        tmpf = rs[i]['tmpf']
        mph = rs[i]['sknt0'] / 1.18
        psun = pcsun[int(rs[i]['sk'])]
        phour = rs[i]['p'] * 25.4
        relh = mesonet.relh(rs[i]['tmpf'], rs[i]['dwpf'])
        if (relh == "M"):
            relh = 65
        while ((now + mx.DateTime.RelativeDateTime(hours=1)) < ts):
            now += mx.DateTime.RelativeDateTime(hours=1)
            #print 'MISSING', now
            missing += 1
            out.write(fmt %
                      (now.strftime("%Y%m%d%H"), tmpf, mph, psun, phour, relh))

        out.write(fmt %
                  (ts.strftime("%Y%m%d%H"), tmpf, mph, psun, phour, relh))

        now = ts
out.close()
print 'Total missing:', missing
示例#6
0
import mx.DateTime
data = {}
sts = mx.DateTime.DateTime(2010,7,1)
ets = mx.DateTime.DateTime(2010,8,17)
interval = mx.DateTime.RelativeDateTime(days=1)

now = sts
while now < ets:
  data[now.strftime("%Y%m%d")] = [0]*24
  now += interval

rs = asos.query("SELECT valid, tmpf, dwpf from t2010 WHERE station = 'DSM' and valid > '2010-07-01' ORDER by valid ASC").dictresult()
for i in range(len(rs)):
  ts = mx.DateTime.strptime(rs[i]['valid'][:16], '%Y-%m-%d %H:%M')
  h = mesonet.heatidx(rs[i]['tmpf'], mesonet.relh(rs[i]['tmpf'], rs[i]['dwpf']))
  data[ ts.strftime("%Y%m%d") ][ ts.hour ] = h

sts = mx.DateTime.DateTime(2010,7,1)
ets = mx.DateTime.DateTime(2010,8,17)
interval = mx.DateTime.RelativeDateTime(days=1)

now = sts
while now < ets:
  lkp = now.strftime("%Y%m%d")
  sz = 24.0
  cln = []
  for v in data[lkp]:
    if v != 0:
      cln.append(v)
  print "%s,%.2f,%.2f,%.2f" % (now.strftime("%Y-%m-%d"), max(cln), sum( cln ) / float(len(cln)), min(cln) )
示例#7
0
文件: asos2hcd.py 项目: akrherz/MSDOT
now = mx.DateTime.DateTime(1972,12,31,23)
for yr in range(1973,2007):
  sql = "SELECT *, \
   case when sknt > 0 THEN sknt ELSE 0 END as sknt0,\
   case when p01m > 0 THEN p01m ELSE 0 END as p,\
   case when skyc > -1 THEN skyc ELSE 0 END as sk from t%s WHERE station = '%s' and tmpf > -50 and extract(year from valid) = %s ORDER by valid ASC" % (yr,stid,yr)
  rs = asos.query(sql).dictresult()
  for i in range(len(rs)):
    ts = mx.DateTime.strptime(rs[i]['valid'][:13], "%Y-%m-%d %H")
    if (now == ts):
      #print 'DUP', now
      continue
    tmpf = rs[i]['tmpf']
    mph = rs[i]['sknt0'] / 1.18
    psun = pcsun[ int(rs[i]['sk']) ]
    phour = rs[i]['p'] * 25.4
    relh = mesonet.relh( rs[i]['tmpf'], rs[i]['dwpf'])
    if (relh == "M"):
      relh = 65
    while ((now + mx.DateTime.RelativeDateTime(hours=1)) < ts):
      now += mx.DateTime.RelativeDateTime(hours=1)
      #print 'MISSING', now
      missing += 1
      out.write( fmt % (now.strftime("%Y%m%d%H"),tmpf, mph, psun, phour, relh))

    out.write(fmt % (ts.strftime("%Y%m%d%H"), tmpf, mph, psun, phour, relh))

    now = ts
out.close()
print 'Total missing:', missing