Author: Antony Johnston
Publisher: Image Comics
ISBN:
Category : Comics & Graphic Novels
Languages : en
Pages : 32
Book Description
"CHASING SHADOWS" THE CONCLUSION TO BOOK ONE! Rascal runs from the Redguard's clutches-but it will cost her more than she can imagine! Where can she go? Who can she trust? Are you sure? Because nothing seems certain any more. And by the end of this issue, nobody will be above suspicion!
Umbral #6
Author: Antony Johnston
Publisher: Image Comics
ISBN:
Category : Comics & Graphic Novels
Languages : en
Pages : 32
Book Description
"CHASING SHADOWS" THE CONCLUSION TO BOOK ONE! Rascal runs from the Redguard's clutches-but it will cost her more than she can imagine! Where can she go? Who can she trust? Are you sure? Because nothing seems certain any more. And by the end of this issue, nobody will be above suspicion!
Publisher: Image Comics
ISBN:
Category : Comics & Graphic Novels
Languages : en
Pages : 32
Book Description
"CHASING SHADOWS" THE CONCLUSION TO BOOK ONE! Rascal runs from the Redguard's clutches-but it will cost her more than she can imagine! Where can she go? Who can she trust? Are you sure? Because nothing seems certain any more. And by the end of this issue, nobody will be above suspicion!
Sunspot Umbral Spectra in the Regions 1925 to 2226 and 2392 to 3480 Cm−1 (2.87 to 4.18 and 4.48 to 5.35 [mu] M)
Author: Lloyd Wallace
Publisher:
ISBN:
Category : Solar photosphere
Languages : en
Pages : 152
Book Description
Publisher:
ISBN:
Category : Solar photosphere
Languages : en
Pages : 152
Book Description
Diccionario Manual Enciclopédico Ilustrado de la Lengua Castellana...
Author: Saturnino Calleja y Fernandez
Publisher:
ISBN:
Category : Spanish language
Languages : en
Pages : 2004
Book Description
Publisher:
ISBN:
Category : Spanish language
Languages : en
Pages : 2004
Book Description
Method for the Calculation of Spacecraft Umbra and Penumbra Shadow Terminator Points
Author: Carlos R. Ortiz Longo
Publisher:
ISBN:
Category : Orbits
Languages : en
Pages : 40
Book Description
A method for calculating orbital shadow terminator points is presented. The current method employs the use of an iterative process which is used for an accurate determination of shadow points. This calculation methodology is required, since orbital perturbation effects can introduce large errors when a spacecraft orbits a planet in a high altitude and/or highly elliptical orbit. To compensate for the required iteration methodology, all reference frame change definitions and calculations are performed with quaternions. Quaternion algebra significantly reduces the computational time required for the accurate determination of shadow terminator points.
Publisher:
ISBN:
Category : Orbits
Languages : en
Pages : 40
Book Description
A method for calculating orbital shadow terminator points is presented. The current method employs the use of an iterative process which is used for an accurate determination of shadow points. This calculation methodology is required, since orbital perturbation effects can introduce large errors when a spacecraft orbits a planet in a high altitude and/or highly elliptical orbit. To compensate for the required iteration methodology, all reference frame change definitions and calculations are performed with quaternions. Quaternion algebra significantly reduces the computational time required for the accurate determination of shadow terminator points.
The sun seen with the atacama large mm and sub-mm array (ALMA) - first results
Author: Costas E Alissandrakis
Publisher: Frontiers Media SA
ISBN: 2832525067
Category : Science
Languages : en
Pages : 200
Book Description
Publisher: Frontiers Media SA
ISBN: 2832525067
Category : Science
Languages : en
Pages : 200
Book Description
Sunspot Umbral Spectra in the Region 4000 to 8640 Cm−1 (1.16 to 2.50 [microns])
Author: Lloyd Wallace
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 282
Book Description
Publisher:
ISBN:
Category : Spectrum, Solar
Languages : en
Pages : 282
Book Description
Sunspots: Theory and Observations
Author: J.H. Thomas
Publisher: Springer Science & Business Media
ISBN: 9401127697
Category : Science
Languages : en
Pages : 422
Book Description
This volume contains the invited papers presented at the NATO Advanced Research Workshop on the Theory of Sunspots, held in Cambridge, England, 22-27 September 1991. The idea of holding this Workshop first arose during the Solar Optical Telescope work shop on Theoretical Problems in High-Resolution Solar Physics in Munich in 1985. At that meeting, separate discussion groups were formed to consider specific topics in solar physics. The discussion group on sunspots recommended that there be a meeting devoted to theoretical problems associated with sunspots, the motivation being the consensus that theory seemed to lag behind the observational evidence in our quest for a satisfactory un derstanding of the physics of sunspots. This recommendation was warmly received and the two of us were designated to organize the Workshop. Although the Workshop eventually took place later than originally envisioned, the de lay turned out to be fortunate and the timing of the Workshop was ideal for a number of reasons. There have been remarkable improvements in high-resolution observations of sunspots in the past few years, and many important new observational results were pre sented for the first time at this Workshop (by groups working at the Lockheed Palo Alto Research Laboratories, the Swedish and German telescopes in the Canary Islands, and the V. S. National Solar Observatory). Vector magnetographs and Stokes polarimetry have at last given us reliable measurements of the vector magnetic fields in sunspots.
Publisher: Springer Science & Business Media
ISBN: 9401127697
Category : Science
Languages : en
Pages : 422
Book Description
This volume contains the invited papers presented at the NATO Advanced Research Workshop on the Theory of Sunspots, held in Cambridge, England, 22-27 September 1991. The idea of holding this Workshop first arose during the Solar Optical Telescope work shop on Theoretical Problems in High-Resolution Solar Physics in Munich in 1985. At that meeting, separate discussion groups were formed to consider specific topics in solar physics. The discussion group on sunspots recommended that there be a meeting devoted to theoretical problems associated with sunspots, the motivation being the consensus that theory seemed to lag behind the observational evidence in our quest for a satisfactory un derstanding of the physics of sunspots. This recommendation was warmly received and the two of us were designated to organize the Workshop. Although the Workshop eventually took place later than originally envisioned, the de lay turned out to be fortunate and the timing of the Workshop was ideal for a number of reasons. There have been remarkable improvements in high-resolution observations of sunspots in the past few years, and many important new observational results were pre sented for the first time at this Workshop (by groups working at the Lockheed Palo Alto Research Laboratories, the Swedish and German telescopes in the Canary Islands, and the V. S. National Solar Observatory). Vector magnetographs and Stokes polarimetry have at last given us reliable measurements of the vector magnetic fields in sunspots.
INTRODUCCION A LA ELECTROCARDI, OGRAFIA
Author: UDO K. LINDNER
Publisher: Springer Science & Business Media
ISBN: 9788407001578
Category : Science
Languages : en
Pages : 508
Book Description
Publisher: Springer Science & Business Media
ISBN: 9788407001578
Category : Science
Languages : en
Pages : 508
Book Description
Solar Surface Magnetism
Author: R. J. Rutten
Publisher: Springer Science & Business Media
ISBN: 940111188X
Category : Science
Languages : en
Pages : 532
Book Description
Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohydrodynamic processes that lead to the multitude of fascinat ing phenomena of solar magnetic activity, and from solar surface observations we must also infer the interplay of convection and magnetism that regulates field dispersal, drives the heating of the outer-atmospheric plasma, and generates the solar wind. There is much to be learned from solar surface magnetism in physics and astrophysics; currently, there are rapid developments in this exciting field. The workshop of which this volume contains the proceedings aimed at a synthesis between observers and theorists, both with regard to the discrete elements that are the building blocks of solar magnetism and with regard to the larger-scale spatial and temporal patterns in which the magnetic elements emerge and disappear. The workshop was held during November 1-5, 1993 in Soesterberg, The Netherlands. The fifty participants took a very active part in making the workshop quite a lively one. The articles in these proceedings cover most of the oral and poster presentations, excepting a dozen soon to be published elsewhere.
Publisher: Springer Science & Business Media
ISBN: 940111188X
Category : Science
Languages : en
Pages : 532
Book Description
Observations of the solar magnetic field are largely confined to the radiation emitted from the photosphere, the thin layer of the solar atmosphere which we call "the solar surface". It is from solar surface observations that we must infer the internal structure and the internal magnetohydrodynamic processes that lead to the multitude of fascinat ing phenomena of solar magnetic activity, and from solar surface observations we must also infer the interplay of convection and magnetism that regulates field dispersal, drives the heating of the outer-atmospheric plasma, and generates the solar wind. There is much to be learned from solar surface magnetism in physics and astrophysics; currently, there are rapid developments in this exciting field. The workshop of which this volume contains the proceedings aimed at a synthesis between observers and theorists, both with regard to the discrete elements that are the building blocks of solar magnetism and with regard to the larger-scale spatial and temporal patterns in which the magnetic elements emerge and disappear. The workshop was held during November 1-5, 1993 in Soesterberg, The Netherlands. The fifty participants took a very active part in making the workshop quite a lively one. The articles in these proceedings cover most of the oral and poster presentations, excepting a dozen soon to be published elsewhere.
Proceedings of the Royal Society of London
Author: Royal Society (Great Britain)
Publisher:
ISBN:
Category : Electronic journals
Languages : en
Pages : 662
Book Description
Obituary notices of deceased fellows were included in v. 7-64; v. 75 is made up of "obituaries of deceased fellows, chiefly for the period 1898-1904, with a general index to previous obituary notices"; the notices have been continued in subsequent volumes as follows: v. 78a, 79b, 80a-b- 86a-b, 87a 88a-b.
Publisher:
ISBN:
Category : Electronic journals
Languages : en
Pages : 662
Book Description
Obituary notices of deceased fellows were included in v. 7-64; v. 75 is made up of "obituaries of deceased fellows, chiefly for the period 1898-1904, with a general index to previous obituary notices"; the notices have been continued in subsequent volumes as follows: v. 78a, 79b, 80a-b- 86a-b, 87a 88a-b.