adsabs/AstroCLIMB huggingface dataset:
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Posterior distributions for the STABLE+SMBHB strings models including the SMBHB parameters A BHB and γ BHB. We also report the marginalized ﹩{\mathrm{log}}_{10}G\mu ﹩ posterior distributions for the STABLE string models (blue lines).
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Same as Figure 8, but including the spectral shape parameters a, b, c and SMBHB parameters A BHB and γ BHB.
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Same as in Figure 5, but for the PT-SOUND (left panel) and PT-BUBBLE models with a low-frequency slope fixed to the value predicted by causality, i.e., a = 3.
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Same as Figure 12, but including the spectral shape parameters b, c and the SMBHB parameters A BHB and γ BHB.
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Same as Figure 10, but including the SMBHB parameters A BHB and γ BHB.
Paper: The NANOGrav 15 yr Data Set: Search for Signals from New Physics
Authors: Adeela Afzal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Paul T. Baker, Bence Bécsy, Jose Juan Blanco-Pillado, Laura Blecha, Kimberly K. Boddy, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, Maria Charisi, Shami Chatterjee, Katerina Chatziioannou, Belinda D. Cheeseboro, Siyuan Chen, Tyler Cohen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kathryn Crowter, Curt J. Cutler, Megan E. DeCesar, Dallas DeGan, Paul B. Demorest, Heling Deng, Timothy Dolch, Brendan Drachler, Richard von Eckardstein, Elizabeth C. Ferrara, William Fiore, Emmanuel Fonseca, Gabriel E. Freedman, Nate Garver-Daniels, Peter A. Gentile, Kyle A. Gersbach, Joseph Glaser, Deborah C. Good, Lydia Guertin, Kayhan Gültekin, Jeffrey S. Hazboun, Sophie Hourihane, Kristina Islo, Ross J. Jennings, Aaron D. Johnson, Megan L. Jones, Andrew R. Kaiser, David L. Kaplan, Luke Zoltan Kelley, Matthew Kerr, Joey S. Key, Nima Laal, Michael T. Lam, William G. Lamb, T. Joseph W. Lazio, Vincent S. H. Lee, Natalia Lewandowska, Rafael R. Lino dos Santos, Tyson B. Littenberg, Tingting Liu, Duncan R. Lorimer, Jing Luo, Ryan S. Lynch, Chung-Pei Ma, Dustin R. Madison, Alexander McEwen, James W. McKee, Maura A. McLaughlin, Natasha McMann, Bradley W. Meyers, Patrick M. Meyers, Chiara M. F. Mingarelli, Andrea Mitridate, Jonathan Nay, Priyamvada Natarajan, Cherry Ng, David J. Nice, Stella Koch Ocker, Ken D. Olum, Timothy T. Pennucci, Benetge B. P. Perera, Polina Petrov, Nihan S. Pol, Henri A. Radovan, Scott M. Ransom, Paul S. Ray, Joseph D. Romano, Shashwat C. Sardesai, Ann Schmiedekamp, Carl Schmiedekamp, Kai Schmitz, Tobias Schröder, Levi Schult, Brent J. Shapiro-Albert, Xavier Siemens, Joseph Simon, Magdalena S. Siwek, Ingrid H. Stairs, Daniel R. Stinebring, Kevin Stovall, Peter Stratmann, Jerry P. Sun, Abhimanyu Susobhanan, Joseph K. Swiggum, Jacob Taylor, Stephen R. Taylor, Tanner Trickle, Jacob E. Turner, Caner Unal, Michele Vallisneri, Sonali Verma, Sarah J. Vigeland, Haley M. Wahl, Qiaohong Wang, Caitlin A. Witt, David Wright, Olivia Young, Kathryn M. Zurek
Figure caption: Same as Figure 11, but including the SMBHB parameters A BHB and γ BHB.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: (a), (b) Solar wind radial magnetic field (B R ) and speed (V  R ) during 2021 November 19–21. (c) Proton energy flux vs. energy. (d), (e), (f), (g), (h) The top axis indicates the PSP solar radial distance (au). Ion composition during November 19–21. Spectrograms for iron (Fe), oxygen (O), helium (3He, 4He), and protons (H). (i) GOES soft X-ray flux profile (1–8 Å, 1 s cadence) during November 19–21.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Microstream periodicities in four intervals on 2021 November 19 and 20. Left: (a) Solar wind radial speed (V  R ) in Interval #2. (b) The smoothed and detrended light curve after subtracting the red trend shown in (a) from the original V  R . (c) Wavelet power spectrum of the detrended signal. Red contours outline the 99% significance level. (d) Global wavelet power spectrum. The dashed line is the 99% global confidence level. Right: same methods as in the left panels but for Interval #3.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Jetlets at the base of a plume in CH1 on 2021 November 20. Top row: AIA 304, 171, and 193 Å images of the plume. Remaining rows: zoomed views of the base in the same AIA channels. Arrows point to the footpoint brightenings and associated jetlets propagating along plumelets. An animation of this figure is available at doi:10.5281/zenodo.7924233. The animation runs from 01:01:35 UT to 11:57:23 UT. The real-time duration is 79 s.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: (a) PSP position on 2021 November 20, 12:00 UT. (b) PFSS extrapolation on November 20, 12:04 UT. White (pink) color marks closed (open) field lines. (c), (d) PSP footpoint connectivity to CH1 (AIA 193 Å and photospheric magnetogram synoptic map) on November 20, 12:00 UT. PSP was connected to CH1 on November 19–20 and to CH2 on November 21.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: AIA 193 Å light curves and wavelet plots for the region shown in panel (b) for four intervals on 2021 November 20, using the same methods as in Figure 3.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Microstream periodicities in two intervals on 2021 November 21. Same methods as in Figure 3. Left: Interval #4. Right: Interval #6.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Microstream periodicities in Interval 1 on 2021 November 19 and Intervals 2, 4, and 5 on 2021 November 20, using the same methods as in Figure 3.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: (a), (b) AIA 171 and 193 Å images of CH1 on 2021 November 20. (c) Zoomed view of the white box in (a). Jets are marked by arrows. (d) HMI magnetogram (B = ±10 G) of the white box in (a). Green (blue) is positive (negative) polarity. (e), (g) AIA 171 Å image of recurrent jets (marked by arrow) from the bright point in CH1 marked by a blue arrow in (c). N = null point. (f) Same image as in (e) overlaid by HMI LOS field-strength contours (B = ±10 G). Jet is marked by an arrow. (h) Potential field extrapolation of the jet source showing the fan-spine magnetic topology. Yellow (red) field lines are closed (open). The animations showing parts of this figure are available at doi:10.5281/zenodo.7924233. The first animation (1) shows the AIA 171 Å and HMI magnetogram images with a larger field of view (FOV). The second animation (2) shows the AIA 171 Å and magnetogram images of a smaller FOV. The first and second parts are similar to panels (c) and (d). The third animation (3) shows HMI magnetogram contours (±10 G) overlaid on 171 Å images. This is similar to panels (e) and (f). All three of these animations run from November 19, 20:12:45 UT to November 20, 22:41:15 UT. The real-time duration for all these three animations is 53 s. The fourth animation (4) shows the AIA 171 Å images of recurrent jets from the bright point in CH1 marked by a blue arrow in panel (c), overlaid by HMI magnetogram contours (±10 G). This animation runs from 01:00:45 UT to 12:05:09 UT on November 20. The real-time duration for this animation is 30 s.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Microstream periodicities in Interval 6 on 2021 November 20 and Intervals 1–3 on November 21, using the same methods as in Figure 3.
Paper: New Evidence on the Origin of Solar Wind Microstreams/Switchbacks
Authors: Pankaj Kumar, Judith T. Karpen, Vadim M. Uritsky, Craig E. Deforest, Nour E. Raouafi, C. Richard DeVore, Spiro K. Antiochos
Figure caption: Microstream periodicities in Intervals 5, 7, and 8 on 2021 November 21, using the same methods as in Figure 3.
Paper: Discovery and Timing Analysis of New Pulsars in Globular Cluster NGC 5024: New Observations from FAST
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, P. C. C. Freire, Shuo Cao, Lei Qian
Figure caption: Acceleration model for M53. The black solid lines represent the upper and lower limits for the line-of-sight accelerations (a  ℓGC) caused by the cluster as a function of the total angular offset from the center of the cluster (θ ⊥). The triangles represent independent upper limits for the pulsar accelerations along the line of sight, ﹩{a}_{{\ell },{\rm{P}},\max }﹩. The limit for M53A, from Y. Lian et al. (2023, in preparation), is well above the upper limit of this figure. The vertical dashed line represents the core radius. The cluster model can account for the negative ﹩\dot{P}﹩ values of M53B and E. The remaining pulsars are above that prediction, which is allowed because a  u  has a contribution from their intrinsic spin period derivatives, which are positive.
Paper: Discovery and Timing Analysis of New Pulsars in Globular Cluster NGC 5024: New Observations from FAST
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, P. C. C. Freire, Shuo Cao, Lei Qian
Figure caption: Positions of M53A–E and six X-ray sources in M53, marked with red stars and circles, respectively. The center of M53 is shown as a blue plus sign. The position of M53A is from Y. Lian et al. (2023, in preparation). The blue circles in the middle show a core radius (0.′35) and a half-light radius (1.′31). The background is the X-ray image of M53 from the Chandra X-ray Observatory archive (ObsID 6560). The left panel displays the details. For reference, the beam size of FAST is 3′.
Paper: Discovery and Timing Analysis of New Pulsars in Globular Cluster NGC 5024: New Observations from FAST
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, P. C. C. Freire, Shuo Cao, Lei Qian
Figure caption: Integrated pulse profiles by summing all detections. All profiles are for 64 bins.
Paper: JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region
Authors: D. Harsono, P. Bjerkeli, J. P. Ramsey, K. M. Pontoppidan, L. E. Kristensen, J. K. Jørgensen, H. Calcutt, Z-Y. Li, A. Plunkett
Figure caption: Comparison between 12CO (4.65 μm) and H I (1.87 μm) normalized spectra.
Paper: Discovery and Timing Analysis of New Pulsars in Globular Cluster NGC 5024: New Observations from FAST
Authors: Yujie Lian, Zhichen Pan, Haiyan Zhang, P. C. C. Freire, Shuo Cao, Lei Qian
Figure caption: Timing residuals from the best-fit timing models presented in Table 2 as a function of the observation date for M53B–E.
Paper: A Model for Confined Solar Eruptions Including External Reconnection
Authors: Jun Chen, Xin Cheng, Bernhard Kliem, MingDe Ding
Figure caption: Initial configurations of the simulations. (a) Bipole case, q 2 = 0. (b) Quadrupole1 case with q 2 = − 4 × 1013 T m2. The blue field line is the magnetic axis, the transparent yellow tube shows the toroidal current channel. (c)–(e) Distributions of squashing factor Q in the plane y = 0, characterizing the magnetic topology, including Quadrupole2. (f) n(R) of the external field excluding the field from the rope, plotted vs. height z = R − d; dashed lines mark the heights where n(R) → ± ∞ , which are lower than the heights of the corresponding upper X-lines in panels (d) and (e).
Paper: A Model for Confined Solar Eruptions Including External Reconnection
Authors: Jun Chen, Xin Cheng, Bernhard Kliem, MingDe Ding
Figure caption: Height–time (upper), velocity–time (middle) and acceleration–time (lower) profiles of the apex point of the flux rope axis in the three runs. The run Bipole (green profiles) is scaled with the green t-axis, other runs are scaled with the black t-axis.