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99 captures
9 Apr 16 - 2 Aug 24
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ALMA Solar Ephemeris Generator
Select user interface
GUI (by clicking on the solar image)
Text (manual input of coordinates)
Input FITS file
File:
AIA image (local)
AIA synoptic 94 (latest)
AIA synoptic 131 (latest)
AIA synoptic 171 (latest)
AIA synoptic 193 (latest)
AIA synoptic 211 (latest)
AIA synoptic 304 (latest)
AIA synoptic 335 (latest)
AIA synoptic 1600 (latest)
AIA synoptic 1700 (latest)
AIA synoptic 4500 (latest)
AIA image (for testing)
Date:
-
Size:
-
x
-
Format:
-
View header
Visualization
Scaling function:
linear
sqrt
cuberoot
log
sqrtlog
loglog
Color:
gray
heat
A
B
Frame
<
>
of
0
.
Show grid
Stonyhurst
Carrington
helioprojective
Show ALMA 12m beam size in band:
Band 3
Band 4
Band 5
Band 6
Band 7
Band 8
Band 9
Band 10
cursor (wcs) = (-, -), intensity = -
Pointing
Reference date:
HPC X:
HPC Y:
arcsec
Sun distance:
m
P:
B0:
L0:
deg
Get from JPL Horizons
Pointing
Pixel (x, y)
Helioprojective (x, y)
arcsec
Heliographic (CMD, B)
degrees
Heliographic (L, B)
degrees
Mosaic observation
Width:
arcsec
Height:
arcsec
Angle:
degrees
Estimated min. no. of pointings for ALMA 12m array is 1 (single pointing).
Location
Change default location (ALMA)
ALMA (Chile)
VLA (USA)
Nobeyama (Japan)
SSRT (Russia)
MUSER (China)
Geocenter
User specified
Lat. (N):
Lon. (E):
Alt.:
m
Observation
Start of observation (UT):
End of observation (UT):
Step size (minutes):
Differential rotation profile:
Don't use (Earth synchronized rotation)
No rotation
Solid rotation (Carrington)
Sunspot groups (Sudar et al., 2014)
H-alpha filaments (Brajša et al., 1991)
Coronal bright points (Wöhl et al., 2010)
User specified
A:
B:
C:
deg/day
Height above photosphere (km):
Generate ephemeris
Show original JPL file
Show ephemeris table
Download table data
Status window: