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position_n.pro
: To calculate the pole angle ($\theta$ ) for a given time of observation. -
timestamp.pro
: position_n.pro internally depends on this function to get time stamp string. -
hour_angle.pro
: position_n.pro use this function to calculate Hour Angle of the sun if approx keyword is set.
This file (CSV: Download Here; TXT: Download Here) contains following information
- Col 1: Filename as stored in KoSO archive, It may varies from one version to another.
- Col 2: Corrected Time of observation (Tobs)
- Col 3: Flag, specifying the correctness of Tobs (Correct 0; Incorrect 1; Unknown -1; Bad 2). Here, Bad implies that the data quality is too bad and our algorithm has failed to get the Tobs.
- Col 4: Pole angle calculated using the Equation 1 and 2 of the article.
Will be updated soon
These files (Plage: Download Here; Sunspot: Download Here))
- Col 1: Year of observation over which data is used to calculate latitudinal extent.
-
Col 2: First Quartile (
$Q1$ ), representing latitude below which 25% plage/sunspot area is covered. -
Col 3: Second Quartile (
$Q2$ ), representing the median latitude of plage/sunspot area distribution for given year. -
Col 4: Thirdt Quartile (
$Q3$ ), representing latitude below which 75% or latitude above which 25% plage/sunspot area is covered.