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Astronomy & Astrophysics manuscript no. H3984 March 20, 2003 (DOI: will be inserted by hand later)
 

Summary: Astronomy & Astrophysics manuscript no. H3984 March 20, 2003
(DOI: will be inserted by hand later)
Simultaneous observations of solar transition region blinkers and
explosive events by SUMER, CDS and BBSO
Are blinkers, explosive events and spicules the same phenomenon?
M.S. Madjarska and J.G. Doyle
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland
Abstract. The SoHO discovery of the new `blinker' phenomena focused our study on the search of its relation to already known
phenomena such as explosive events and spicules. The study was performed using a specially planned joint observing program
involving the Coronal Diagnostic Spectrometer (CDS), Solar Ultraviolet Measurements of Emitted Radiation spectrograph
(SUMER) and Big Bear Solar Observatory (BBSO) magnetograph. Within each blinker, the SUMER data reveal the presence
of small­scale (3 ## --5 ## ), short­lived (2­3 min) bright features not seen in the CDS data which has sometimes being interpreted as
oscillations in SUMER data. With this data we have clearly identified UV explosive events in CDS data. The explosive events
show a size close to the small­scale brightenings forming the blinker core. However, they appear in the SUMER data with their
typical strong blue and red wings while the blinker shows at best only a small increase in the emission of the blue and red wings
and in most instances the typical transition region red­shift in the center of the line. In all cases the explosive events cover one
pixel in CDS corresponding to a size of 4 ## × 4 ## --6 ## . All identified explosive events were located at the border of the bright
network i.e. the blinker, in the network or even in the internetwork. From this data, we believe that blinkers and explosive events
are two separate phenomena not directly related or triggering each other. In this study, the Doppler shift was derived in a blinker
phenomenon for the first time. It ranges from --5 to 25 km s -1 and is predominantly red­shifted. The observed magnetic flux

  

Source: Armagh Observatory

 

Collections: Physics