. KP are available via the WWW and FTP according to Rules of the Road . The Interball-Tail KP archive is final. All data are also available in CDAWeb. Latest changes (27 October 2003) . WWW Data retrieval . Data avalability plots . KP list . Full KP description . Archive structure and access (FTP and local) . INTERBALL-TAIL PIs and contacts . IDL plotting routines . Author: Anatoli Petrukovich, IKI RAN . Questions and comments are welcomed at apetruko@iki.rssi.ru

List of available intervals . ... 00012823.ITB 28-01-00 23:41 01-02-00 13:02 2305.0k . ... 00032916.ITB 29-03-00 16:06 02-04-00 04:59 2349.4k . 00040210.ITB 02-04-00 10:05 03-04-00 07:28 547.2k . ... 00050118.ITB 01-05-00 18:19 02-05-00 13:45 548.1k . ... 00050613.ITB 06-05-00 13:56 10-05-00 03:54 2305.2k . ... 00061312.ITB 13-06-00 12:02 17-06-00 02:37 2354.6k . ... 00062816.ITB 28-06-00 16:08 02-07-00 06:59 2394.0k . ... 00072901.ITB 29-07-00 01:00 01-08-00 15:44 2353.2k . ...

... The spacecraft payload included magnetic field, plasma wave, and particle instruments that were built with broad international cooperation; many European, Canadian, and Cuban institutions participated. ... In particular, multi-spacecraft observations help to study sub-storms--bursty releases of energy that accumulate in the Earth's magnetotail when the interplanetar y magnetic field AND Fig. ... Peak energy and local east-west magnetic field variations (Interball-Auroral) are compared. ...

Large-scale wave processes in space plasma. ... G.V.Lizunov, O.P. Verkhoglyadova, and K.I. Churyumov, Plasma- beam instabilities in comatary ionospheres, Russian Astronomical Journ. ... Verkhoglyadova, O.P., V.V. Grimalsky, Propagation of ion- sound solitons in unhomogeneous plasma, Ukrainian Phys. Journ., ... Verkhoglyadova, O.P., Ivchenko, V.N., Plasma regime identification technique using magnetospheric satellite measurements, Space Sci. and Technology, 4 (5/6), 18-27 (1998) (in Ukrainian). ...

... 1, 2010 Table 3 Best-fit Parameters of the Spectral Analysis of PCA and HEXTE Observation of SS 433 in 3­150 keV Energy Rangea Observational ID 10127-01-01-00 10127-01-02-00 10127-01-03-00 10127-01-04-00 10127-01-05-00 10127-01-06-00 10127-01 ... 1.39(1) 1.13(1) 0.99(1) 1.07(1) 0.98(4) 1.17(1) 1.15(3) 1.17(1) 1.21(3) 1.25(6) 1.06(2) 1.09(4) 1.23(1) 1.20(5) 1.07(7) log(A)b 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 ... Softening of X-ray spectra is seen when the Figure 2. ...