The document appears to be a catalog from the website www.paschalia-flowers.com consisting of 38 pages. Each page references the website and does not contain any other visible text or images.
ALMA will deliver exciting opportunities to advance our understanding of solar prominences and filaments, and constrain models of prominence fine structures.
The document provides information about studying physics and astronomy at the University of Glasgow. It discusses Glasgow's location in Scotland, the university's colleges and schools, research areas and facilities in physics and astronomy, undergraduate and postgraduate degree programs, funding options, student life, and fees for international students. The university has a strong reputation for research and teaching in physics and astronomy.
The document appears to be a catalog from the website www.paschalia-flowers.com consisting of 38 pages. Each page references the website and does not contain any other visible text or images.
ALMA will deliver exciting opportunities to advance our understanding of solar prominences and filaments, and constrain models of prominence fine structures.
The document provides information about studying physics and astronomy at the University of Glasgow. It discusses Glasgow's location in Scotland, the university's colleges and schools, research areas and facilities in physics and astronomy, undergraduate and postgraduate degree programs, funding options, student life, and fees for international students. The university has a strong reputation for research and teaching in physics and astronomy.
Plasma diagnostic in eruptive prominences from SDO/AIA observations at 304 ÅUniversity of Glasgow
The document discusses plasma diagnostic observations of eruptive solar prominences from SDO/AIA at 304 Angstroms. New non-LTE radiative transfer calculations allow plasma parameters like temperature, column mass, and radial velocity to vary, unlike previous models. The observations and new models show that the Helium II 304 Angstrom line intensity can either decrease or increase with increasing radial velocity, depending on changes in the plasma parameters. Allowing parameters to vary produces a range of intensities that matches the range seen in SDO/AIA observations qualitatively.
The document appears to be a catalog from a flower shop website called www.paschalia-flowers.com that includes different flower arrangements for civil weddings. It lists the website URL repeated across multiple pages from 39-57 but does not include any other details about specific arrangements.
We present SOPRA (Solar Off-limb Prominence Reconstruction Algorithm), an algorithm
which automatically detects prominences above the limb in EUV images taken in the He II
channel at 304 A and subsequently reconstructs the structures to extract their morphological parameters.
SOPRA determines the characteristics of radial intensity profiles outward from the limb and
uses Support Vector Machines in order to classify them as belonging to prominence or other
structures. Pixels detected as belonging to a prominence are then used as the starting point
to reconstruct the whole object by morphological image processing techniques.
The algorithm is applied to the entire SOHO/EIT data set and a catalogue of detected
prominences is produced. We present the initial statistical analysis of this catalogue, and
discuss its use for solar prominence research and for space weather monitoring.
We also assess the performance of SOPRA when applied to SDO/AIA images.
Solar spectroscopy is the study of the sun's spectrum of light. Important early developments included Newton observing the sun's spectrum using a prism in 1704, and Fraunhofer describing the dark absorption lines in 1817. Now high resolution spectroscopy is used to determine properties of the sun's atmosphere from the photosphere to the corona, and observe phenomena like solar flares. It provides insights into the sun's structure and energy transport mechanisms.
This document appears to be a listing of web pages from www.paschalia-flowers.com, ranging from page 58 to page 79. Each entry simply lists the URL for the page number given. The document does not contain any other text or context.
Plasma diagnostic in eruptive prominences from SDO/AIA observations at 304 ÅUniversity of Glasgow
The document discusses plasma diagnostic observations of eruptive solar prominences from SDO/AIA at 304 Angstroms. New non-LTE radiative transfer calculations allow plasma parameters like temperature, column mass, and radial velocity to vary, unlike previous models. The observations and new models show that the Helium II 304 Angstrom line intensity can either decrease or increase with increasing radial velocity, depending on changes in the plasma parameters. Allowing parameters to vary produces a range of intensities that matches the range seen in SDO/AIA observations qualitatively.
The document appears to be a catalog from a flower shop website called www.paschalia-flowers.com that includes different flower arrangements for civil weddings. It lists the website URL repeated across multiple pages from 39-57 but does not include any other details about specific arrangements.
We present SOPRA (Solar Off-limb Prominence Reconstruction Algorithm), an algorithm
which automatically detects prominences above the limb in EUV images taken in the He II
channel at 304 A and subsequently reconstructs the structures to extract their morphological parameters.
SOPRA determines the characteristics of radial intensity profiles outward from the limb and
uses Support Vector Machines in order to classify them as belonging to prominence or other
structures. Pixels detected as belonging to a prominence are then used as the starting point
to reconstruct the whole object by morphological image processing techniques.
The algorithm is applied to the entire SOHO/EIT data set and a catalogue of detected
prominences is produced. We present the initial statistical analysis of this catalogue, and
discuss its use for solar prominence research and for space weather monitoring.
We also assess the performance of SOPRA when applied to SDO/AIA images.
Solar spectroscopy is the study of the sun's spectrum of light. Important early developments included Newton observing the sun's spectrum using a prism in 1704, and Fraunhofer describing the dark absorption lines in 1817. Now high resolution spectroscopy is used to determine properties of the sun's atmosphere from the photosphere to the corona, and observe phenomena like solar flares. It provides insights into the sun's structure and energy transport mechanisms.
This document appears to be a listing of web pages from www.paschalia-flowers.com, ranging from page 58 to page 79. Each entry simply lists the URL for the page number given. The document does not contain any other text or context.