{"id":17,"date":"2019-03-15T18:06:07","date_gmt":"2019-03-15T18:06:07","guid":{"rendered":"http:\/\/sites.epss.ucla.edu\/jweygand\/?page_id=17"},"modified":"2019-03-15T18:14:16","modified_gmt":"2019-03-15T18:14:16","slug":"17-2","status":"publish","type":"page","link":"https:\/\/sites.epss.ucla.edu\/jweygand\/17-2\/","title":{"rendered":"Weimer et al. [2003] Propagated Solar Wind"},"content":{"rendered":"\n<p>Curator: James Weygand <br>\nInstitute of Geophysics and Planetary Physics, UCLA<br>\nPhone: (310) 825-3547 <br>\nE-mail: jweygand(at)igpp.ucla.edu<\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Location:<\/h2>\n\n\n\n<p><a href=\"http:\/\/vmo.igpp.ucla.edu\/data1\/Weygand\/\">http:\/\/vmo.igpp.ucla.edu\/data1\/Weygand\/<\/a><\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Reference:<\/h2>\n\n\n\n<p>Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C.W. Smith, and J. Watermann, Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, <a href=\"https:\/\/agupubs.onlinelibrary.wiley.com\/doi\/full\/10.1029\/2002JA009405\">DOI:10.1029\/2002JA009405<\/a>, 2003.<\/p>\n\n\n\n<h2 class=\"wp-block-heading\">The Code:<\/h2>\n\n\n\n<p>The original IDL code was provide by Dan Weimer. James Weygand has ported the code into a Matlab routine. If you want the code<a href=\"mailto:jweygand@igpp.ucla.edu\"> E-mail James Weygand.<\/a><\/p>\n\n\n\n<h2 class=\"wp-block-heading\">The Data<\/h2>\n\n\n\n<p>Nearly all the data was obtained from Coordinated Data Analysis Web (CDAWeb). Some data was obtained directly from the PIs. Processed and propagated solar wind data available at: The Heliophysics Data Environment.<\/p>\n\n\n\n<h2 class=\"wp-block-heading\">Propagated Solar Wind Data Availability at 1 min resolution.<\/h2>\n\n\n\n<TABLE BORDER=2>\n   <TR>\n\t<TD ><B>Spacecraft    <\/B> <\/TD>\n\t<TD ><B>Available Data<\/B> <\/TD>\n\t<TD ><B>Coordinate System    <\/B> <\/TD>\n\t<TD ><B>Acknowledgement<\/B> <\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ACE<\/TD>\n\t<TD > MFI data    Feb. 1998 to Feb. 2018 <BR> \n              SWEPAM data Feb. 1998 to Feb. 2018 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  ACE\/MFI data C. Smith <BR> ACE\/SWEPAM data D. McComas<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > Geotail <\/TD>\n\t<TD > MGF data  Oct. 1993 to July 2018 <BR> \n              LEP data  Oct. 1993 to July 2018 <BR>\n              CPI data  Oct. 1992 to 2016 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  Geotail\/MGF data S. Kokubun <BR> Geotail\/LEP data T. Mukai<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > IMP 8 <\/TD>\n\t<TD > MAG data Nov. 1973 to Jun. 2000 <BR> \n              PLA data Nov. 1973 to Jun. 2000 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> IMP 8\/MAG data A. Szabo <BR> IMP 8\/PLA data A. Lazarus<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ISEE 1 <\/TD>\n\t<TD > Magnetometer data Oct. 1977 to Jan. 1984<BR> \n              SWE data          Oct. 1977 to Jan. 1984 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  ISEE 1\/Magnetometer data C.T. Russell <BR>  ISEE 1\/SWE data J.T. Gosling<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ISEE 3 <\/TD>\n\t<TD > MAG data     Aug. 1978 to Feb. 1980 <BR> \n              Plasma data  Aug. 1978 to Feb. 1980 <BR> <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> ISEE 3\/MAG data E.J. Smith <BR> ISEE 3\/Solar Wind Plasma data J.T. Gosling<\/TD>\n   <\/TR>\n   \n   <TR>\n\t<TD > Wind <\/TD>\n\t<TD > MFI data Jan. 1995 to Apr. 2018 <BR> \n              SWE data Jan. 1995 to Apr. 2018 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> Wind\/MFI data R. Lepping <BR> Wind\/SWE data K. Ogilvie <BR> Wind\/3DP data R. Lin<\/TD>\n   <\/TR>\n   <TR>\n   <\/TR>\n<\/TABLE>\n\n\n\n<h2 class=\"wp-block-heading\">Non-propagated Solar Wind Data Availability at 1 min resolution.<\/h2>\n\n\n\n<TABLE BORDER=2>\n   <TR>\n\t<TD ><B>Spacecraft    <\/B> <\/TD>\n\t<TD ><B>Available Data<\/B> <\/TD>\n\t<TD ><B>Coordinate System    <\/B> <\/TD>\n\t<TD ><B>Acknowledgement<\/B> <\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ACE<\/TD>\n\t<TD > MFI data    Sept. 1997 to Feb. 2018 <BR> \n              SWEPAM data Feb. 1998 to Feb. 2018 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  ACE\/MFI data C. Smith <BR> ACE\/SWEPAM data D. McComas<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > Geotail <\/TD>\n\t<TD > MGF data  Sept. 1992 to July 2018 <BR> \n              LEP data  Oct. 1993 to July 2018 <BR>\n              CPI data  Oct. 1993 to 2016 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  Geotail\/MGF data S. Kokubun <BR> Geotail\/LEP data T. Mukai<\/TD>\n   <\/TR>\n   <TR>        \n\t<TD > IMP 8 <\/TD>\n\t<TD > MAG data Nov. 1973 to Jun. 2000 <BR> \n              PLA data Nov. 1973 to Jun. 2000 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> IMP 8\/MAG data A. Szabo <BR> IMP 8\/PLA data A. Lazarus<\/TD>\n   <\/TR>\n   <TR>        \n\t<TD > Interball <\/TD>\n\t<TD > FGM-I data Aug. 1995 to Oct. 2000  <\/TD>\n\t<TD > GSE <\/TD>\n\t<TD> Interball\/FGM-I data  J. Rustenbach <\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ISEE 1 <\/TD>\n\t<TD > Magnetometer data Oct. 1977 to Jan. 1984<BR> \n              SWE data          Oct. 1977 to Jan. 1984 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  ISEE 1\/Magnetometer data C.T. Russell <BR>  ISEE 1\/SWE data J.T. Gosling<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ISEE 2 <\/TD>\n\t<TD > Magnetometer data Oct. 1977 to Jan. 1982<BR> \n              SWE data          Aug. 1978 to Sept. 1978 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD>  ISEE 1\/Magnetometer data C.T. Russell <BR>  ISEE 1\/SWE data J.T. Gosling<\/TD>\n   <\/TR>\n   <TR>\n\t<TD > ISEE 3 <\/TD>\n\t<TD > MAG data     Aug. 1978 to Dec. 1982 <BR> \n              Plasma data  Aug. 1978 to Feb. 1980 <BR> <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> ISEE 3\/MAG data E.J. Smith <BR> ISEE 3\/Solar Wind Plasma data J.T. Gosling<\/TD>\n   <\/TR>\n   \n   <TR>\n\t<TD > Wind <\/TD>\n\t<TD > MFI data Jan. 1995 to Apr. 2018 <BR> \n              SWE data Jan. 1995 to Apr. 2018 <\/TD>\n\t<TD > GSM\/GSE <\/TD>\n\t<TD> Wind\/MFI data R. Lepping <BR> Wind\/SWE data K. Ogilvie <BR> Wind\/3DP data R. Lin<\/TD>\n   <\/TR>\n   <TR>\n   <\/TR>\n<\/TABLE>\n\n\n\n<h2 class=\"wp-block-heading\">Acknowledgments<\/h2>\n\n\n\n<p>If you use any of the above data please be sure to acknowledge Dan Weimer for providing the Weimer variance analysis routine.<\/p>\n\n\n\n<p>Questions or Corrections can be directed to : jweygand(at)igpp.ucla.edu <br>\nReturn to the top James&#8217; Research Page<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Curator: James Weygand Institute of Geophysics and Planetary Physics, UCLA Phone: (310) 825-3547 E-mail: jweygand(at)igpp.ucla.edu Location: http:\/\/vmo.igpp.ucla.edu\/data1\/Weygand\/ Reference: Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C.W. Smith, and J. Watermann, Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, DOI:10.1029\/2002JA009405, 2003. The [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-17","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/pages\/17","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/comments?post=17"}],"version-history":[{"count":2,"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/pages\/17\/revisions"}],"predecessor-version":[{"id":20,"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/pages\/17\/revisions\/20"}],"wp:attachment":[{"href":"https:\/\/sites.epss.ucla.edu\/jweygand\/wp-json\/wp\/v2\/media?parent=17"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}