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Name:

sum_hor_mag_grad.pro

Purpose:

Calculates the sum of the horizontal magnetic field and the separation distance between the leading and the following polarity subgroups 

Calling sequence:

sum_hor_mag_grad,c_img_blos,c_img_cont,g_s,slf,d_l_f,weight_cent,lead_cent,foll_cent,fit_coeff=fit_coeff,minsize=minsize

Input parameters:

c_img_blos : Blos HARP cutout magnetogram, corrected for limb presence and deproject.

c_img_blos : continuum HARP image, corrected for limb presence.

Keywords:

fit_coeff: The coefficients K1 and K2 for the empirical relation <B>=f(A) (see Korsós et al. 2014)

Min_size : minimum size of detected umbra (in MSH). Default equal to 0.5 (in accordance with the Debrecen Observatory limit)

Output:

g_s: The sum of the horizontal magnetic gradient according to Korsos & Erdelyi (2016)

slf: the seperation distance

d_l_f: the distance between leading and following

weight_cent: the weighted centroid

lead_cent: weighted centroid of the leading subgroup

foll_Cent: weighet centroid of the following subgroup


Property name in DB:

gs_slf.g_s, gs_slf.slf, gs_slf.d_l_f, gs_slf.weight_cent, gs_slf.lead_cent, gs_slf.foll_cent, gs_slf.fit_coeff

Repository:

https://dev.flarecast.eu/stash/projects/FE/repos/gs_slf-idl/browse

References:

 

M. B. Korsós et al. 2014 The Astrophysical Journal,  789, 107

 

M. B. Korsós et al. 2015 The Astrophysical Journal Letters, 802 L21 

M. B. Korsós and R. Erdélyi 2016 ApJ 823 153

Padinhatteeri et al. 2016, Solar Physics, 291, 41

 

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