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- Sofort-KaufenKreuzkalibrierung von fernen UV-Spektren von Objekten des Sonnensystems und der Heliosphäre
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eBay-Artikelnr.:364702661026
Artikelmerkmale
- Artikelzustand
- ISBN-13
- 9781493947096
- Type
- NA
- Publication Name
- NA
- ISBN
- 9781493947096
- Book Title
- Cross-Calibration of Far Uv Spectra of Solar System Objects and the Heliosphere
- Book Series
- Issi Scientific Report Ser.
- Publisher
- Springer New York
- Item Length
- 9.2 in
- Publication Year
- 2016
- Format
- Trade Paperback
- Language
- English
- Illustrator
- Yes
- Item Height
- 0.6 in
- Genre
- Science
- Topic
- Spectroscopy & Spectrum Analysis, Physics / Astrophysics, Astronomy
- Item Weight
- 152.9 Oz
- Item Width
- 6.1 in
- Number of Pages
- VII, 275 Pages
Über dieses Produkt
Product Identifiers
Publisher
Springer New York
ISBN-10
1493947095
ISBN-13
9781493947096
eBay Product ID (ePID)
240069384
Product Key Features
Book Title
Cross-Calibration of Far Uv Spectra of Solar System Objects and the Heliosphere
Number of Pages
VII, 275 Pages
Language
English
Topic
Spectroscopy & Spectrum Analysis, Physics / Astrophysics, Astronomy
Publication Year
2016
Illustrator
Yes
Genre
Science
Book Series
Issi Scientific Report Ser.
Format
Trade Paperback
Dimensions
Item Height
0.6 in
Item Weight
152.9 Oz
Item Length
9.2 in
Item Width
6.1 in
Additional Product Features
Intended Audience
Trade
Series Volume Number
13
Number of Volumes
1 vol.
Table Of Content
Distribution of interstellar H atoms in the heliosphere and backscattered solar Lyman-α.- Solar parameters for modeling interplanetary background.- 30 Years of Interplanetary Background Data: A Global View.- Lyman-alpha Models from Messenger and SOHO data.- New Horizons Cruise Observations of Lyα Emissions from the Interplanetary Medium.- A New Catalog of Ultraviolet Stellar Spectra.- Absolute Ultraviolet Irradiance of the Moon from SORCE SOLSTICE.- Lyman-alpha Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWAN.
Synopsis
This book discusses various fields of Far UV spectroscopy, ranging from a catalog of stellar spectra to detailed modeling and measurements of the interplanetary background. It presents various types of data sets and different techniques for calibration., Distribution of interstellar H atoms in the heliosphere and backscattered solar Lyman-.- Solar parameters for modeling interplanetary background.- 30 Years of Interplanetary Background Data: A Global View.- Lyman-alpha Models from Messenger and SOHO data.- New Horizons Cruise Observations of Ly Emissions from the Interplanetary Medium.- A New Catalog of Ultraviolet Stellar Spectra.- Absolute Ultraviolet Irradiance of the Moon from SORCE SOLSTICE.- Lyman-alpha Observations of Comet Holmes from SORCE SOLSTICE and SOHO SWAN., This book is the result of a working group sponsored by ISSI in Bern, which was initially created to study possible ways to calibrate a Far Ultraviolet (FUV) instrument after launch. In most cases, ultraviolet instruments are well calibrated on the ground, but unfortunately, optics and detectors in the FUV are very sensitive to contaminants and it is very challenging to prevent contamination before and during the test and launch sequences of a space mission. Therefore, ground calibrations need to be confirmed after launch and it is necessary to keep track of the temporal evolution of the sensitivity of the instrument during the mission. The studies presented here cover various fields of FUV spectroscopy, including a catalog of stellar spectra, datasets of Moon Irradiance, observations of comets and measurements of the interplanetary background. Detailed modelling of the interplanetary background is presented as well. This work also includes comparisons of older datasets with current ones. This raises the question of the consistency of the existing datasets. Previous experiments have been calibrated independently and comparison of the datasets may lead to inconsistencies. The authors have tried to check that possibility in the datasets and when relevant suggest a correction factor for the corresponding data.", This book is the result of a working group sponsored by ISSI in Bern, which was initially created to study possible ways to calibrate a Far Ultraviolet (FUV) instrument after launch. In most cases, ultraviolet instruments are well calibrated on the ground, but unfortunately, optics and detectors in the FUV are very sensitive to contaminants and it is very challenging to prevent contamination before and during the test and launch sequences of a space mission. Therefore, ground calibrations need to be confirmed after launch and it is necessary to keep track of the temporal evolution of the sensitivity of the instrument during the mission. The studies presented here cover various fields of FUV spectroscopy, including a catalog of stellar spectra, datasets of Moon Irradiance, observations of comets and measurements of the interplanetary background. Detailed modelling of the interplanetary background is presented as well. This work also includes comparisons of older datasets with current ones. This raises the question of the consistency of the existing datasets. Previous experiments have been calibrated independently and comparison of the datasets may lead to inconsistencies. The authors have tried to check that possibility in the datasets and when relevant suggest a correction factor for the corresponding data.
LC Classification Number
QB500.5-785
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