iPhoneAlle anzeigen
iPhone 11iPhone 11 ProiPhone 11 Pro MaxiPhone 12iPhone 12 ProiPhone 12 Pro MaxiPhone 12 miniiPhone 13iPhone 13 ProiPhone 13 Pro MaxiPhone 13 miniiPhone 14iPhone 14 PlusiPhone 14 ProiPhone 14 Pro MaxiPhone 15iPhone 15 PlusiPhone 15 ProiPhone 15 Pro MaxiPhone 16iPhone 16 PlusiPhone 16 ProiPhone 16 Pro MaxiPhone 16eiPhone 8iPhone 8 PlusiPhone SE 2020iPhone SE 2022iPhone XiPhone XRiPhone XSiPhone XS Max
Galaxy A-SerieAlle anzeigen
Galaxy A12Galaxy A13Galaxy A13 5GGalaxy A14Galaxy A15Galaxy A16Galaxy A17 5GGalaxy A20eGalaxy A21Galaxy A22Galaxy A23Galaxy A24Galaxy A25Galaxy A26 5GGalaxy A32Galaxy A33Galaxy A34Galaxy A35Galaxy A36 5GGalaxy A40Galaxy A41Galaxy A42Galaxy A50Galaxy A51Galaxy A52Galaxy A53Galaxy A54Galaxy A55Galaxy A56 5GGalaxy A70Galaxy A71Galaxy A72
Redmi SeriesAlle anzeigen
Redmi 10Redmi 13CRedmi 15 5GRedmi Note 10Redmi Note 10 ProRedmi Note 11Redmi Note 11 ProRedmi Note 11 Pro Plus 5GRedmi Note 11sRedmi Note 12Redmi Note 12 5GRedmi Note 12 ProRedmi Note 12 Pro 5GRedmi Note 12 Pro PlusRedmi Note 13Redmi Note 13 5GRedmi Note 13 ProRedmi Note 13 Pro PlusRedmi Note 14Redmi Note 14 Pro PlusRedmi Note 8Redmi Note 8 ProRedmi Note 9Redmi Note 9 Pro
- Startseite
Bücher Englische Bücher Wissen & Bildung Naturwissenschaft, Medizin, Informatik, Technik Physik & Astronomie Astronomie Diagnostic of the solar transition region and corona from VUV spectroscopy and imaging
Derzeit nicht verfügbar
Handgeprüfte Gebrauchtware
Bis zu 50 % günstiger als neu
Der Umwelt zuliebe
Diagnostic of the solar transition region and corona from VUV spectroscopy and imaging
Neda Dadashi (Broschiert, Englisch)
★★★★★
☆☆☆☆☆ Keine Bewertungen vorhanden
Optischer Zustand
Beschreibung
Imaging and spectroscopy at vacuum ultra-violet (VUV: 100 to 2000 Å) wavelengths are the key tools to study the outer solar atmosphere. This is a very dynamic environment where structures and their changes can be observed down to very small scales. However, it also shows average properties that must be accounted for by any reliable modelling effort. The average Doppler shift shown by spectral… lines formed from chromosphere to corona, in particular, reveals important information on the mass and energy balance of the solar atmosphere, providing a tight observational constraint on any model of the solar corona. So far, spectroscopic studies revealed a persistent average red shift of the lines formed at temperatures below 0.5 MK that revert to blue shift at higher temperatures. However, for temperatures above 1 MK the behaviour was, so far, unknown.
Since VUV radiation is entirely absorbed by the atmosphere of the Earth, it can only be detected with instruments operating in space. In this thesis I have used simultaneous and co-spatial VUV spectra recorded by two spectrometers: SUMER (Solar Ultraviolet Measurements of Emitted Radiation)/SoHO (Solar and Heliospheric Observatory) and EIS (Extreme ultraviolet Imaging Spectrometer)/Hinode. The behaviour of the absolute Doppler shift versus temperature (up to 2 MK) is measured by using a novel technique developed during this thesis work and applied to the quiet Sun near disk center and to the moss area of an active region. The results are compared with different coronal models present in the literature. Dieses Produkt haben wir gerade leider nicht auf Lager.
Handgeprüfte Gebrauchtware
Bis zu 50 % günstiger als neu
Der Umwelt zuliebe
Technische Daten
Erscheinungsdatum
17.07.2013
Sprache
Englisch
EAN
9783942171748
Herausgeber
Uni-Edition
Sonderedition
Nein
Autor
Neda Dadashi
Seitenanzahl
128
Auflage
1
Einbandart
Broschiert
Schlagwörter
Sun, SUMER/SoHO, solar, Sonne, Astronomie, Max-Planck-Institut, EIS/Hinode
Höhe
210 mm
Breite
14.8 cm
-.-
★★★★★
☆☆☆☆☆ Leider noch keine Bewertungen
Leider noch keine Bewertungen
Sicher bei rebuy kaufen
Schreib die erste Bewertung für dieses Produkt!
Wenn du eine Bewertung für dieses Produkt schreibst, hilfst du allen Kund:innen, die noch überlegen, ob sie das Produkt kaufen wollen. Vielen Dank, dass du mitmachst!
Sicher bei rebuy kaufen