Search Results - "Pietarila, A."

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  1. 1

    Comparison of Ground-Based and Space-Based Longitudinal Magnetograms by Pietarila, A., Bertello, L., Harvey, J. W., Pevtsov, A. A.

    Published in Solar physics (2013)
    “…We compare photospheric line-of-sight magnetograms from the Synoptic Optical Long-term Investigations of the Sun (SOLIS) Vector Spectro-Magnetograph (VSM)…”
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    Journal Article
  2. 2

    Kink Waves in an Active Region Dynamic Fibril by Pietarila, A, Cuadrado, R. Aznar, Hirzberger, J, Solanki, S. K

    Published in The Astrophysical journal (01-10-2011)
    “…We present high spatial and temporal resolution Ca II 8542 A observations of a kink wave in an on-disk chromospheric active region fibril. The properties of…”
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    Journal Article
  3. 3

    Ca II 854.2 nm BISECTORS AND CIRCUMFACULAR REGIONS by Pietarila, A, Harvey, J W

    Published in The Astrophysical journal (20-02-2013)
    “…Active regions appear bright in Ca II 854.2 nm line core intensity while the surrounding areas, referred to as circumfacular regions, are darker than the…”
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    Journal Article
  4. 4

    SYNOPTIC MAPPING OF CHROMOSPHERIC MAGNETIC FLUX by Jin, C L, Harvey, J W, Pietarila, A

    Published in The Astrophysical journal (10-03-2013)
    “…We used daily full-disk Ca II 854.2 nm magnetograms from the Synoptic Optical Long Term Investigations of the Sun (SOLIS) facility to study the chromospheric…”
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    Journal Article
  5. 5

    SIGNATURE OF DIFFERENTIAL ROTATION IN SUN-AS-A-STAR Ca II K MEASUREMENTS by BERTELLO, L, PEVTSOV, A. A, PIETARILA, A

    Published in The Astrophysical journal (10-12-2012)
    “…The characterization of solar surface differential rotation (SDR) from disk-integrated chromospheric measurements has important implications for the study of…”
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    Journal Article
  6. 6

    SOLAR CYCLE VARIATION IN SUN-AS-A-STAR Ca II 854.2 nm BISECTORS by Pietarila, A, Livingston, W

    Published in The Astrophysical journal (01-08-2011)
    “…The bisector of the strong chromospheric Ca II 854.2 nm line has an inverse-C shape, the cause of which is not yet fully understood. We show that the amplitude…”
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    Journal Article
  7. 7

    Constructing Semi-Empirical Sunspot Models for Helioseismology by Cameron, R. H., Gizon, L., Schunker, H., Pietarila, A.

    Published in Solar physics (01-02-2011)
    “…One goal of helioseismology is to determine the subsurface structure of sunspots. In order to do so, it is important to understand first the near-surface…”
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    Journal Article
  8. 8
  9. 9

    Transport of Magnetic Flux from the Canopy to the Internetwork by Pietarila, A, Cameron, R. H, Danilovic, S, Solanki, S. K

    Published in The Astrophysical journal (10-03-2011)
    “…Recent observations have revealed that 8% of linear polarization patches in the internetwork (INW) quiet Sun are fully embedded in downflows. These are not…”
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    Journal Article
  10. 10

    Spectropolarimetric Observations of the Ca II lambda 8498 and lambda 8542 in the Quiet Sun by Pietarila, A, Socas-Navarro, H, Bogdan, T

    Published in The Astrophysical journal (10-07-2007)
    “…The Ca II infrared triplet is one of the few magnetically sensitive chromospheric lines available for ground-based observations. We present spectropolarimetric…”
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    Journal Article
  11. 11
  12. 12

    Simulation of Quiet-Sun Waves in the Ca II Infrared Triplet by Pietarila, A, Socas-Navarro, H, Bogdan, T, Carlsson, M, Stein, R. F

    Published in The Astrophysical journal (01-04-2006)
    “…The Ca II infrared triplet lines around 8540 Ae are good candidates for observing chromospheric magnetism. Model spectra of these lines are obtained by…”
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  13. 13
  14. 14

    SIGNATURE OF DIFFERENTIAL ROTATION IN SUN-AS-A-STAR Can II MEASUREMENTS by Bertello, L, PEVTSOV, A A, Pietarila, A

    Published in The Astrophysical journal (10-12-2012)
    “…The characterization of solar surface differential rotation (SDR) from disk-integrated chromospheric measurements has important implications for the study of…”
    Get full text
    Journal Article
  15. 15

    Instrumental and Observational Artifacts in Quiet Sun Magnetic Flux Cancellation Functions by Pietarila, A., Pietarila Graham, J.

    Published in Solar physics (01-02-2013)
    “…Under the assumption that the photospheric quiet Sun magnetic field is turbulent, the cancellation function has previously been used to estimate the true,…”
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    Journal Article
  16. 16

    KINK WAVES IN AN ACTIVE REGION DYNAMIC FIBRIL by Pietarila, A., Cuadrado, R. Aznar, Hirzberger, J., Solanki, S. K.

    Published in The Astrophysical journal (01-10-2011)
    “…We present high spatial and temporal resolution Ca II 8542 A observations of a kink wave in an on-disk chromospheric active region fibril. The properties of…”
    Get full text
    Journal Article
  17. 17

    Constructing Semi-Empirical Sunspot Models forHelioseismology by Cameron, R H, Gizon, L, Schunker, H, Pietarila, A

    Published in Solar physics (01-02-2011)
    “…One goal of helioseismology is to determine the subsurface structure of sunspots. In order to do so, it is important to understand first the near-surface…”
    Get full text
    Journal Article
  18. 18

    Spectropolarimetric Inversions of the Ca II 8498 and 8542 AA Lines in the Quiet Sun by Pietarila, A, Socas-Navarro, H, Bogdan, T

    Published in The Astrophysical journal (20-11-2007)
    “…We study non-LTE inversions of the Ca II infrared triplet lines as a tool for inferring physical properties of the quiet Sun. The inversion code is successful…”
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    Journal Article
  19. 19

    On the Formation of the Resonance Lines of Helium in the Sun by Pietarila, Anna, Judge, Philip G

    Published in The Astrophysical journal (10-05-2004)
    “…To investigate the cause of anomalously bright resonance lines of helium in the Sun, we have studied the magnitude of the enhancements and some proposals made…”
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  20. 20

    Spectropolarimetric Observations of the Ca II l8498 and l8542 in the Quiet Sun by Pietarila, A, Socas-Navarro, H, Bogdan, T

    Published in The Astrophysical journal (10-07-2007)
    “…The Ca II infrared triplet is one of the few magnetically sensitive chromospheric lines available for ground-based observations. We present spectropolarimetric…”
    Get full text
    Journal Article