======================================================================= Oersted Newsletter #10, 1999 (January 28) ======================================================================= Table of Contents ======================================================================= 1. Oersted Launch Delayed 2. Oersted Internal Field Science ======================================================================= ----------------------------------------------------------------------- 1. Oersted Launch Delayed ----------------------------------------------------------------------- From: Kim Bisgaard (kib@dmi.dk) As you may know, the launch of ARGOS, SUNSAT, and OERSTED has been scrubbed again. The delay this time is due to an on launch pad engine cutoff. Initial investigation shows that the cutoff was due to low pressure in the fuel tank of a steering engine. NOT due to the weather this time! There will be at meeting in the morning California time to decide a new launch date. ----------------------------------------------------------------------- 2. Oersted Internal Field Science ----------------------------------------------------------------------- From: Nils Olsen (nio@dsri.dk) Dear Colleagues, As mentioned in the Oersted Newsletter #6/99, I agreed to take over the task of Oersted Main Field Modeling and coordination of the Internal Field Science in general. This is, of course, a great challenge, and I look forward to an exciting and fruitful collaboration. IN-FLIGHT CALIBRATION AND INITIAL FIELD MODELS One of the most important issues is be to obtain a reliable in-flight calibration of the magnetometer as a first step for providing you with the high-quality data you are expecting. Getting experience with the behavior of the magnetometer in space, and how to calibrate it, will therefore have high priority during the next weeks and months. We have asked Terry Sabaka (NASA/GSFC) to visit Copenhagen and help us in this effort. He has agreed to come about two months after launch for six weeks. During this period we will work on the in-flight calibration of the vector magnetometer (combined estimation of main field model and magnetometer parameters) as well as on the Oersted IGRF candidate. The decision on the calibration parameters to be used will be made by a calibration sub-group based on the results of in-flight calibration algorithms. There are plans for a meeting of the group a few weeks after launch. I'll send you more information on this meeting as soon as we have decided on the date; everybody is welcome to participate in this meeting. It has been suggested to publish the first Oersted Main Field Models with the Oersted Main Field Investigators as co-authors. A first step in this direction was the submission of an abstract for the IAGA meeting in Birmingham. The deadline for abstract submission was January 15, and Terry will present the Oersted IGRF candidate at the IAGA meeting. Let's hope that the satellite will be launched soon and that the data are as good as we expect. The text of the submitted abstract: AN IGRF 2000 CANDIDATE MODEL BASED UPON OERSTED SATELLITE DATA T.J. Sabaka (Raytheon ITSS Corp., Lanham, MD 20706, USA, email: sabaka@linus.gsfc.nasa.gov) Oersted Main Field Working Group The Danish satellite Oersted, launched in January 1999, is to provide the best sampling of the geomagnetic field for main field modelling purposes since the Magsat mission of 1980. An IGRF 2000 candidate model, derived from this high-precision vector data set and supplemental observatory measurements, will be presented. SELECTION OF DATA FOR THE MODELING EFFORTS There are plans for selecting/compiling special data sets for the internal field modeling efforts. These data sets will be accumulated in batches of about one month, and are anticipated to contain about 3000 data points (consisting of time, position and the 3 magnetic vector components). The data will be pre-selected according to geomagnetic indices, but the final selection will of course be made after visual inspection, and a good geographical coverage will be taken care of. -----------------------------------------------------------------------