;+ ; Magnetopause crib sheet ; ; do you have suggestions for this crib sheet? ; please send them to clrussell@igpp.ucla.edu ; ; ; $LastChangedBy: clrussell $ ; $LastChangedDate: 2016-05-25 14:40:54 -0700 (Wed, 25 May 2016) $ ; $LastChangedRevision: 21203 $ ; $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/projects/elf/examples/basic/mms_load_state_crib.pro $ ;- pro crib_magnetopause ; Initialize themis settings thm_init ;; ========= ;; mpause_2 ;; ========= ;This magnetopause subroutine calculates the magnetopause (X,Y) locations based on ; the Fairfield model (JGR, 1971). Aberation of 4 degrees is assumed ; The output is the location of the magnetopause down to a very large distance (xmp_max=-300 Re) mpause_2,xmp,ymp xrange=[100, -300] plot, xmp, ymp, xrange=xrange stop ;; ============ ;; mpause_t96 ;; ============ ;This magnetopause subroutine the pressure-dependent magnetopause that is ;used in the T96_01 MODEL ; (TSYGANENKO, JGR, V.100, P.5599, 1995; ESA SP-389, P.181, O;T. 1996) ; AUTHOR: N.A. TSYGANENKO ; INPUT: PD - THE SOLAR WIND RAM PRESSURE IN NANOPAS ; XGSM, YGSM, ZGSM - position of points in re for flagging ; ; OUTPUT: XMGNP, YMGNP, ZMGNP - location of magnetopause in re ; ID - flag, whether XGSM, YGSM, ZGSM are inside or outside mp ; DISTAN - distance between XGSM, YGSM, ZGSM and Xmp0, Ymp0, Zmp0 in re ; Xmp0, Ymp0, Zmp0 is the boundary point, having the same value of TAU ; ; RATIO OF PD TO THE AVERAGE PRESSURE, ASSUMED EQUAL TO 2 nPa: ; set date and time ; download data for 8/2/2015 date = '2019-01-05/00:00:00' timespan,date,1,/day tr=timerange() dynp=2. re=6378. thm_load_state, probe='d', trange=tr, datatype='pos' cotrans,'thd_state_pos','thd_state_pos_gse',/gei2gse cotrans,'thd_state_pos_gse','thd_state_pos_gsm',/gse2gsm get_data, 'thd_state_pos_gsm', data=pos_gsm mpause_t96,dynp,xmgnp=xmgnp,ymgnp=ymgnp,xgsm=pos_gsm.y[*,0]/re,ygsm=pos_gsm.y[*,1]/re,zgsm=pos_gsm.y[*,2]/re,id=id,distan=distan help, id help, distance xrange=[20,-60] plot, xmgnp, ymgnp, xrange=xrange end