The Earth magnetopause is the boundary between magnetosphere and shocked solar wind. Its location shape are primarily determined by properties of wind interplanetary magnetic field (IMF) but nature control parameters to what extent they impact stand-off distance, flaring, symmetries, on dayside night side, still not well known. We present a large statistical study based an extensive multi-missi...

Despite the widespread use of coronary stents and effective anticoagulation regimens, the treatment of ostial lesions is limited by high restenosis rates. Ostial stenosis is a technically difficult condition to treat but this novel technique shows the ability to enable the optimal coverage of the ostium with excellent stent flaring using a Flash ostial balloon (Cardinal Health Inc., Dublin, OH).

VLA continuous monitoring of ER Vul during two 11.5 hour sessions in September 1995 in the radio continuum at 3.6 cm (X-band) showed a variation pattern similar to that observed in 1990 and 1991, but at a lower mean flux level. Simultaneous observations with the EUVE satellite in the 70 – 140 Å band did not show any significant flaring variability of the star.

The precise physical process that triggers solar flares is not currently understood. Here we attempt to capture the signature of this mechanism in solar image data of various wavelengths and use these signatures to predict flaring activity. We do this by developing an algorithm that [1] automatically generates features in 5.5 TB of image data taken by the Solar Dynamics Observatory of the solar...

Variable non-thermal radio emission from Galactic X-ray binaries is a trace of relativistic jets, created near accretion disks. The spectral characteristics of a lot of radio flares in the X-ray binaries with jets (RJXB) is discussed in this report. We carried out several long daily monitoring programs with the RATAN-600 radio telescope of the sources: SS433, Cyg X-3, LS I +61303, GRS 1915+10 a...

A Kerr black hole can flare quasi-periodically, if it is magnetically connected to the accretion disk. The flares extract the rotational energy of the hole. The flaring occurs because the hole twists the magnetic field lines beyond the threshold of the screw instability. Subject headings: black holes – magnetic fields