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PROBLEMS OF GEOCOSMOS

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Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008)<br />

instrumentation complex onboard the CORONAS-F spacecraft. Zhitnik et al. (2003) phenomenologically<br />

described such features as long-living plasma bodies with bright orbed cores, localized at a height of 0.1–0.3<br />

solar radii, and darker legs, probably giant loops, connecting the cores with active regions.<br />

Ulysses spacecraft flied over the poles of the Sun, climbed its maximum latitude of 80.2 degrees North on<br />

31 July 1995 with the last passing on 14 January 2008. Figure 2 shows the decreasing of the temperature<br />

distribution above the solar Polar Regions.<br />

Figure 2. The temperature of the Sun’s polar coronal holes as measured by the SWICS instrument on board Ulysses<br />

(Credit to Ulysses).<br />

Among the numerous results of HINODE let’s look at the X-ray jets which are observed in the solar polar<br />

atmosphere (e.g. Kulhane et al. 2007; Filippov, Golub and Koutchmi 2007; Savcheva 2007). Recent results<br />

(Shimojo<br />

et al. 2007; Shimojo 2008) reveal that over 70% of jets occur in mixed polarity regions and X-ray<br />

jets in the polar coronal hole are not always associated with the kG-patches (kilo Gauss magnetic field).<br />

Some X-ray jets are associated with very weak magnetic field. And, the jets are strongly associated with the<br />

emerging/cancelling magnetic flux.<br />

The series of wonderful EUV images from two satellites with fine resolution of A (head) and B (behind) of<br />

the Solar TErrestrial RElations Observatory<br />

(STEREO) provide 3D reconstruction of the coronal loops<br />

and<br />

corona (Aschwanden et al. 2008a, 2008b).<br />

SOHO (Solar and Heliospheric observatory) is the leader in the list of the space observatories not only<br />

due to the numerous publications; SOHO demonstrates<br />

a successful international collaboration inside the<br />

SOHO<br />

teams and collaborations with other teams among the solar and the heliospheric society.<br />

Birth of the Solar Cycle<br />

"On January 4, 2008, a reversed-polarity sunspot appeared—and this signals the start of Solar Cycle 24"<br />

(David Hathaway of the Marshall<br />

Space Flight Center, HASA deadlines)<br />

Figure 3. Left image: Sun in continuum. Right image: MDI (Michelson Doppler Imager)<br />

magnetogram. White color<br />

shows a positive polarity, black is marked a negative polarity.<br />

35

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