Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'

S. J.González Manrique; C. Denker; C. Kuckein; A. Pastor Yabar; M. Collados; M. Verma; H. Balthasar; A. Diercke; C. E. Fischer; P. Gömöry; N. Bello González; R. Schlichenmaier; M. Cubas Armas; T. Berkefeld; A. Feller; S. Hoch; A. Hofmann; A. Lagg; H. Nicklas; D. Orozco Suárez; D. Schmidt; W. Schmidt; M. Sigwarth; M. Sobotka; S. K. Solanki; D. Soltau; J. Staude; K. G. Strassmeier; R. Volkmer; O. Von Der Lühe; T. Waldmann

doi:10.1017/S1743921317000278

Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'

S. J.González Manrique
, C. Denker
, C. Kuckein
, A. Pastor Yabar
, M. Collados
, M. Verma
, H. Balthasar
, A. Diercke
, C. E. Fischer
, P. Gömöry
, N. Bello González
, R. Schlichenmaier
, M. Cubas Armas
, T. Berkefeld
, A. Feller
, S. Hoch
, A. Hofmann
, A. Lagg
, H. Nicklas
, D. Orozco Suárez

D. Schmidt, W. Schmidt, M. Sigwarth, M. Sobotka, S. K. Solanki, D. Soltau, J. Staude, K. G. Strassmeier, R. Volkmer, O. Von Der Lühe, T. Waldmann

Research output: Contribution to journal › Article › peer-review

Abstract

A new generation of solar instruments provides improved spectral, spatial, and temporal resolution, thus facilitating a better understanding of dynamic processes on the Sun. High-resolution observations often reveal multiple-component spectral line profiles, e.g., in the near-infrared He i 10830 A triplet, which provides information about the chromospheric velocity and magnetic fine structure. We observed an emerging flux region, including two small pores and an arch filament system, on 2015 April 17 with the 'very fast spectroscopic mode' of the GREGOR Infrared Spectrograph (GRIS) situated at the 1.5-meter GREGOR solar telescope at Observatorio del Teide, Tenerife, Spain. We discuss this method of obtaining fast (one per minute) spectral scans of the solar surface and its potential to follow dynamic processes on the Sun. We demonstrate the performance of the 'very fast spectroscopic mode' by tracking chromospheric high-velocity features in the arch filament system.

Original language	English
Pages (from-to)	28-33
Number of pages	6
Journal	Proceedings of the International Astronomical Union
Volume	12
DOIs	https://doi.org/10.1017/S1743921317000278
Publication status	Published - 2016

Bibliographical note

Publisher Copyright:
© International Astronomical Union 2017.

Keywords

Methods: Data analysis
Sun: Chromosphere
Sun: Filaments
Sun: Infrared
Sun: Photosphere
Techniques: Spectroscopic

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10.1017/S1743921317000278

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Manrique, S. J. G., Denker, C., Kuckein, C., Yabar, A. P., Collados, M., Verma, M., Balthasar, H., Diercke, A., Fischer, C. E., Gömöry, P., González, N. B., Schlichenmaier, R., Armas, M. C., Berkefeld, T., Feller, A., Hoch, S., Hofmann, A., Lagg, A., Nicklas, H., ... Waldmann, T. (2016). Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'. Proceedings of the International Astronomical Union, 12, 28-33. https://doi.org/10.1017/S1743921317000278

@article{5ed07eddc375477d9cc403a2681b278f,

title = "Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'",

abstract = "A new generation of solar instruments provides improved spectral, spatial, and temporal resolution, thus facilitating a better understanding of dynamic processes on the Sun. High-resolution observations often reveal multiple-component spectral line profiles, e.g., in the near-infrared He i 10830 A triplet, which provides information about the chromospheric velocity and magnetic fine structure. We observed an emerging flux region, including two small pores and an arch filament system, on 2015 April 17 with the 'very fast spectroscopic mode' of the GREGOR Infrared Spectrograph (GRIS) situated at the 1.5-meter GREGOR solar telescope at Observatorio del Teide, Tenerife, Spain. We discuss this method of obtaining fast (one per minute) spectral scans of the solar surface and its potential to follow dynamic processes on the Sun. We demonstrate the performance of the 'very fast spectroscopic mode' by tracking chromospheric high-velocity features in the arch filament system.",

keywords = "Methods: Data analysis, Sun: Chromosphere, Sun: Filaments, Sun: Infrared, Sun: Photosphere, Techniques: Spectroscopic",

author = "Manrique, \{S. J.Gonz{\'a}lez\} and C. Denker and C. Kuckein and Yabar, \{A. Pastor\} and M. Collados and M. Verma and H. Balthasar and A. Diercke and Fischer, \{C. E.\} and P. G{\"o}m{\"o}ry and Gonz{\'a}lez, \{N. Bello\} and R. Schlichenmaier and Armas, \{M. Cubas\} and T. Berkefeld and A. Feller and S. Hoch and A. Hofmann and A. Lagg and H. Nicklas and Su{\'a}rez, \{D. Orozco\} and D. Schmidt and W. Schmidt and M. Sigwarth and M. Sobotka and Solanki, \{S. K.\} and D. Soltau and J. Staude and Strassmeier, \{K. G.\} and R. Volkmer and \{Von Der L{\"u}he\}, O. and T. Waldmann",

note = "Publisher Copyright: {\textcopyright} International Astronomical Union 2017.",

year = "2016",

doi = "10.1017/S1743921317000278",

language = "English",

volume = "12",

pages = "28--33",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

Manrique, SJG, Denker, C, Kuckein, C, Yabar, AP, Collados, M, Verma, M, Balthasar, H, Diercke, A, Fischer, CE, Gömöry, P, González, NB, Schlichenmaier, R, Armas, MC, Berkefeld, T, Feller, A, Hoch, S, Hofmann, A, Lagg, A, Nicklas, H, Suárez, DO, Schmidt, D, Schmidt, W, Sigwarth, M, Sobotka, M, Solanki, SK, Soltau, D, Staude, J, Strassmeier, KG, Volkmer, R, Von Der Lühe, O & Waldmann, T 2016, 'Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'', Proceedings of the International Astronomical Union, vol. 12, pp. 28-33. https://doi.org/10.1017/S1743921317000278

TY - JOUR

T1 - Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'

AU - Manrique, S. J.González

AU - Denker, C.

AU - Kuckein, C.

AU - Yabar, A. Pastor

AU - Collados, M.

AU - Verma, M.

AU - Balthasar, H.

AU - Diercke, A.

AU - Fischer, C. E.

AU - Gömöry, P.

AU - González, N. Bello

AU - Schlichenmaier, R.

AU - Armas, M. Cubas

AU - Berkefeld, T.

AU - Feller, A.

AU - Hoch, S.

AU - Hofmann, A.

AU - Lagg, A.

AU - Nicklas, H.

AU - Suárez, D. Orozco

AU - Schmidt, D.

AU - Schmidt, W.

AU - Sigwarth, M.

AU - Sobotka, M.

AU - Solanki, S. K.

AU - Soltau, D.

AU - Staude, J.

AU - Strassmeier, K. G.

AU - Volkmer, R.

AU - Von Der Lühe, O.

AU - Waldmann, T.

PY - 2016

Y1 - 2016

N2 - A new generation of solar instruments provides improved spectral, spatial, and temporal resolution, thus facilitating a better understanding of dynamic processes on the Sun. High-resolution observations often reveal multiple-component spectral line profiles, e.g., in the near-infrared He i 10830 A triplet, which provides information about the chromospheric velocity and magnetic fine structure. We observed an emerging flux region, including two small pores and an arch filament system, on 2015 April 17 with the 'very fast spectroscopic mode' of the GREGOR Infrared Spectrograph (GRIS) situated at the 1.5-meter GREGOR solar telescope at Observatorio del Teide, Tenerife, Spain. We discuss this method of obtaining fast (one per minute) spectral scans of the solar surface and its potential to follow dynamic processes on the Sun. We demonstrate the performance of the 'very fast spectroscopic mode' by tracking chromospheric high-velocity features in the arch filament system.

AB - A new generation of solar instruments provides improved spectral, spatial, and temporal resolution, thus facilitating a better understanding of dynamic processes on the Sun. High-resolution observations often reveal multiple-component spectral line profiles, e.g., in the near-infrared He i 10830 A triplet, which provides information about the chromospheric velocity and magnetic fine structure. We observed an emerging flux region, including two small pores and an arch filament system, on 2015 April 17 with the 'very fast spectroscopic mode' of the GREGOR Infrared Spectrograph (GRIS) situated at the 1.5-meter GREGOR solar telescope at Observatorio del Teide, Tenerife, Spain. We discuss this method of obtaining fast (one per minute) spectral scans of the solar surface and its potential to follow dynamic processes on the Sun. We demonstrate the performance of the 'very fast spectroscopic mode' by tracking chromospheric high-velocity features in the arch filament system.

KW - Methods: Data analysis

KW - Sun: Chromosphere

KW - Sun: Filaments

KW - Sun: Infrared

KW - Sun: Photosphere

KW - Techniques: Spectroscopic

UR - https://www.scopus.com/pages/publications/85029923137

U2 - 10.1017/S1743921317000278

DO - 10.1017/S1743921317000278

M3 - Article

AN - SCOPUS:85029923137

SN - 1743-9213

VL - 12

SP - 28

EP - 33

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

ER -

Flows along arch filaments observed in the GRIS 'very fast spectroscopic mode'

Abstract

Bibliographical note

Keywords

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