UCSD IPS Workshop San Diego USA December 18

UCSD IPS Workshop San Diego, USA @ December 18 -20 2016 IPS Common Data Format Munetoshi Tokuamru ISEE, Nagoya University

IPSCDF V 1. 0 • IPSCDF was defined at Nagoya IPS workshop in 2013 (Version 0), and revised at Moleria IPS workshop in 2015 (Version 1. 0). • V 1. 0: addition of the source size • ISEE IPSCDF V 1. 0 data • ftp: //ftp. isee. Nagoya-u. ac. jp/pubvlist/STEL{YYYY}. dat • {YYYY} = Year in JST • Updated on a daily basis • Read-me file • ftp: //ftp. isee. nagoya –u. ac. jp/Read. Me(IPSCDF. v. 1. 0). txt

Read. Me(IPSCDFv. 1. 0). txt STEL(ISEE) IPS data (IPSCDF v. 1. 0) Filename: STELYYYY. dat (YYYY= Year in JST) 1 st line: Header Date Mid. Obs. UT Dur. Site Freq BW Source Size RA-J 2000 Dec-J 2000 Limb Dist. Lat. PA Elong Vel. V-err g-value g-err Method 2 nd and subsequent lines: Data YYMMDD Date in UT i 4. 4, i 2. 2 (1 space) HH: MM: SS Mid-Obs. Time in UT i 2. 2, ': ', i 2. 2 (1 space) MM. M Duration in min f 4. 1 (1 space) STEL Site Code a 4 (1 space) 327 Frequency in MHz i 4 (1 space) 10 Bandwidth in MHz i 2 (1 space) XXXX Source name a 8 (IAU or 3 C catalog) (1 space) -999 Source size in mas (N/A) (1 space) hh mm ss R. A. in J 2000 a 9 (1 x, i 2. 2, 1 x, i 2. 2) (1 space) +dd mm ss Decl. in J 2000 a 9 (i 3, 1 x, i 2. 2) (3 space) X Limb (E or W) a 1 (3 space) FFF. FF P-point heliocentric distance (in solar radii) f 6. 2 (1 space) +FF. F Heliographic p-point latitude (deg) f 5. 1 (1 space) FFF. F PA of P-point (deg) counterclockwise from North f 6. 1 (1 space) FFF. F Elong. angle of LOS (deg) f 5. 1 (1 space) NNNNNN Solar wind speed (km/s) i 6 (-999 if N/A) (1 space) NNNNNN Error estimate of speed (km/s) i 6 (-999 if N/A) (1 space) FF. FFF g-value f 6. 3 (-999 if N/A) (1 space) FF. FFF Error estimate of g-value f 6. 3 (-999 if N/A) (1 space) 3 -St. CC Method a 8 (1 space) -999 Solar wind speed (km/s) (N/A) (1 space) -999 Error estimate of speed (km/s) (N/A) (1 space) FF. FFF g-value f 6. 3 (-999 if N/A) (1 space) FF. FFF Error estimate of g-value f 6. 3 (-999 if N/A) (1 space) 1 -St. PS Method a 8 format(i 4. 4, i 2. 2, 1 x, i 2. 2, ': ', i 2. 2, 1 x, f 4. 1, 1 x, a 4, 1 x, i 2, 1 x, a 8, 1 x, i 4, 1 x, a 9, 3 x, a 1, 3 x, f 6. 2, 1 x, f 5. 1, 1 x, f 6. 1, 1 x, f 5. 1, 1 x, i 6, 1 x, f 6. 3, 1 x, a 8)

Old Format IPS Data VLIST{YY} since 1983 ftp: //ftp. stelab. nagoya-u. ac. jp/pub/vlist The header with 8 lines, followed by {YY} = last 2 digits of year 1 SOURCE Source Name Max. 8 Characters （IAU or ３ C catalog name） 2 YRMNDY Observation Date YYMMDD 3 UT Time HH. H（UT) 4 DIST Distance 小数点以下２桁の実数（AU） 5 HLA Heliocentric Lat. 3 digit integer （degree） 6 HLO Heliocentric Lon. 3 digit integer （degree） 7 GLA Heliographic Lat. 3 digit integer （degree） 8 GLO Heliographic Lon. 3 digit integer （degree） 9 CARR Carrington Rot. 3 digit integer （degree） 10 V Speed 4 digit integer （in km/s） 11 ER Estimation Error 4 digit integer （km/s）, if the error is not available, ER=-999 12 SC-INDX IPS Strength Real number with 3 effective digits （E 10. 3） Obs. Condition Observation Results Coordinates of point-P Note: VLIST_RT is updated on daily basis. ftp: //ftp. stelab. nagoya-u. ac. jp/pub/vlist/rt

Old Format IPS Data VLIST{YY} since 2010 ftp: //ftp. stelab. nagoya-u. ac. jp/pub/vlist/ Added. The same as VLIST except for gvalue in 12 th column instead of IPS strength {YY} = last 2 digits of year Coordinate of Radio Source In B 1950 and J 2000

Old Format IPS Realtime Data ftp: //ftp. stelab. nagoya-u. ac. jp/pub/vlist/rt/ Filename: nagoya. {yyyy} , yyyy=Year This file is updated on daily basis. With no header The same as VLIST except for gvalue in 12 th column instead of IPS strength Coordinate of Radio Source In B 1950 and J 2000