ALMA Solar Ephemeris Generator Tool
Notice to users: For creating ALMA solar proposals (by using ALMA Observing Tool), a dummy ephemeris can be used since it is impossible to know at present time if the desired solar feature will be visible and where on the solar disc, when actual observation takes place. To produce a dummy ephemeris file for a proposal, just click anywhere on the Sun below, then click "Generate ephemeris file for OT" and finally download the file by clicking "Download data below". You can then load that file into your proposal in the Observing Tool. You can even use an already generated sample file, available here .
Input FITS file
File:
AIA image (local)
AIA synoptic 193 (latest)
AIA synoptic 304 (latest)
AIA synoptic 1700 (latest)
Kanzelhohe H-alpha (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 6
Band 7
Band 9
cursor (wcs) = (-, -), intensity = -
Pointing
Observation
Notes
Coordinates of the Sun are astrometric J2000 coordinates from JPL Horizons for the ALMA center of array. Atmospheric refraction is not taken into account.
Physical ephemeris of the Sun are also from JPL Horizons. Note that JPL Horizons gives systematically lower value by ~0.25 degrees in L0 than IMCCE. Values
for P and B0 are the same in both cases to the given accuracy.
Mirror links
Version history
Acknowledgements
AIA synoptic images courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
jsFITS, JavaScript FITS library, https://github.com/slowe/jsFITS
JPL Horizons, http://ssd.jpl.nasa.gov/horizons.cgi
ALMA, http://www.almaobservatory.org
ESO, http://www.eso.org
ALMA Ondrejov ARC node, http://www.asu.cas.cz/alma
Joint Science Operations Center (JSOC), http://jsoc.stanford.edu
Hvar Observatory, http://oh.geof.unizg.hr
Kanzelhöhe Observatory, http://www.kso.ac.at/
References
Brajša, R.; Vršnak, B.; Ruždjak, V.; Schroll, A.; Pohjolainen, S. (1991) Solar differential rotation determined by polar crown filaments. SoPh, 133, p. 195-203.(ADS )
Sudar, D.; Skokić, I.; Ruždjak, D.; Brajša, R.; Wöhl, H. (2014) Tracing sunspot groups to determine angular momentum transfer on the Sun. MNRAS, 439-3, p. 2377-2385.(ADS )
Thompson, W. T. (2006) Coordinate systems for solar image data. A&A, 449-2, p. 791-803.(ADS )
Wöhl, H.; Brajša, R.; Hanslmeier, A.; Gissot, S. F. (2010) A precise measurement of the solar differential rotation by tracing small bright coronal structures in SOHO-EIT images. Results and comparisons for the period 1998-2006. A&A, 520-A29.(ADS )
Created by I. Skokić
Astronomical Institute of the Czech Academy of Sciences Fričova 298, 251 65 Ondřejov, Czech Republic