2007/12/08-10 Hinode Workshop / Hinode 専題研討会 1 XRT Observation Planning R.Kano (NAOJ) and XRT team.

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Presentation transcript:

2007/12/08-10 Hinode Workshop / Hinode 専題研討会 1 XRT Observation Planning R.Kano (NAOJ) and XRT team.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Weekly Meeting On Thursday (JST),  We have a weekly XRT-team meeting via teleconference, and discuss the current status and the next week observations and operations. On Friday (JST),  In a weekly (Hinode team) meeting, XRT-CO (Chief Observer) request and explain the XRT weekly plan, and discuss the Hinode weekly plan with others (SOT-CO, EIS-CO, CP and some experts) based on the results of the monthly meeting. One of the XRT team member is assigned as XRT-CO each week (From Friday to Friday).

Hinode Workshop / Hinode 専題研討会 /12/08-10

Hinode Workshop / Hinode 専題研討会 /12/08-10

Hinode Workshop / Hinode 専題研討会 /12/08-10 Daily Meeting From 10:30JST, the daily meeting starts. In the meeting,  We confirm the Hinode pointing plan for today. If necessary, we can adjust the pointing targets.  We make the Hinode pointing plan for tomorrow. We request the XRT synoptic observation 4 times in a day around 0, 6, 12, and 18 UT. (It can be reduced to 2 times in a day in some cases.)

Hinode Workshop / Hinode 専題研討会 /12/08-10

Hinode Workshop / Hinode 専題研討会 /12/08-10 Hinode Pointing Plan: “re-pointing and tracking schedule” /* re-pointing and tracking schedule */ Fm: 2007/11/28 04:00:00 To: 2007/11/30 11:11:00 /* Date Time Tracking Offset-X Offset-Y */ /* (UT) Curve No. (deg) (deg) */ Latest re-pointing 2007/11/28 00:00: /* Format example, meaningless pointing information : */ AOCS Mem-Upload /11/28 08:43:36 /* Memory upload : # */ ORe-point Start 2007/11/28 10:06: /* 151.5/ : # OP start + 10min, track small emerging region */ ORe-point Start 2007/11/28 10:53: /* 0.0/ 0.0 : synoptic, shifted 47.0 min */ ORe-point Start 2007/11/28 11:03: /* 160.2/ : # Cont. */ ORe-point Start 2007/11/28 17:46: /* 0.0/ 0.0 : synoptic, shifted min */ ORe-point Start 2007/11/28 17:56: /* / 0.0 : # HOP 54, transient horiz fields */ ORe-point Start 2007/11/29 00:01: /* 0.0/ 0.0 : synoptic, shifted 1.0 min */ ORe-point Start 2007/11/29 00:11: /* / 0.0 : # Cont. */ ORe-point Start 2007/11/29 06:00: /* 0.0/ 0.0 : synoptic */ ORe-point Start 2007/11/29 06:10: /* 331.8/ : # Track small emerging region */ ORe-point Start 2007/11/29 10:44: /* 0.0/ 0.0 : Backup plan */ /* End of re-pointing and tracking schedule */ /* AOCS Tracking Parameters before the memory upload */ TR_MEM_ID: /* Track No. Ref-Time of Tracking Helio-long. Helio-lat. Rot. Rate */ /* Date Time(UT) (degree) (degree) (deg/sec) */ Track /11/26 18:00: Track /11/27 10:54: Track /11/22 18:08: Track /11/25 10:43: /* New AOCS Tracking Parameters after the memory upload*/ TR_MEM_ID: Fm: 2007/11/28 10:06:00 /* Track No. Ref-Time of Tracking Helio-long. Helio-lat. Rot. Rate */ /* Date Time(UT) (degree) (degree) (deg/sec) */ Track /11/26 18:00: Track /11/27 10:54: Track /11/22 18:08: Track /11/25 10:43: /* End of Tracking Curve Information */

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Planning XRT-CO makes tomorrow’s plan with COT (Chief Observer Tool).  Prepare XOB (XRT Observation Table).  Create a timeline.  Check the data rate of the timeline. For daily planning, XRT-CO communicates with XRT members, other COs and proposers of observations, if necessary. Here, I explain the outline by using the final product of the COT, a list of XOB and a timeline chart.

Hinode Workshop / Hinode 専題研討会 /12/08-10 A List of XOB

Hinode Workshop / Hinode 専題研討会 /12/08-10 A Timeline Chart

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB) In MDP, 20 PROGrams can be stored. In this test case, 5 PROGrams will be used. XOB#143B and #1460 for Synoptic Obs. XOB#1471 for AR Obs. XOB#1472 for QS Obs. XOB#137B for Backup plan. Only the PROGram which is not stored in MDP will be uploaded with the real-time operation.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation This is a PROGram. One PROGram calls Subroutins up to 8 times. One Subroutin calls Sequences up to 8 times. One Sequence calls exposures up to 8 times.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation FW1 / FW2VL shutterImage TypeExp. DurationRes.FOV size (center)C ompression AECInterval

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation Al-mesh filter images with short (0.5s) & long (8s) exposures, to cover the wider dynamic range.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation Ti-poly filter images with short (1s) & long (16s) exposures.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation A dark image to subtract the CCD bias and dark current.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation A G-band image with opening the visible-light shutter.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation Al-poly filter images with short (0.5s) & long (11s) exposures.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation C-poly filter images with short (1s) & long (16s) exposures.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Synoptic Observation The PROGram #17 runs only once, and then stops. Every Sequence and the Subroutine are called once.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Quiet-Sun Observation

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Quiet-Sun Observation Al-poly, A-poly+Al-mesh, A-poly+Ti-poly, and Ti-poly images with a small FOV are taken with 3 rd set of AEC thresholds.  There are 7 different sets of AEC thresholds. (“0” means disable.) And, a dark image with the same FOV.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Quiet-Sun Observation Al-poly image with a small FOV are taken with 1 st set of AEC thresholds.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): a Quiet-Sun Observation The PROGram #04 continues with endless. The Subroutine #1 is called once in every 10 min*.  The Subroutine #2 is running during this 10 min (=15 x 40 sec). The Subroutine #2 is called once in every 40 sec*.  * The duration becomes long, if exposure durations are elongated by AEC.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): an Active Region Observation Thin-Be, Al-poly, A-poly+Ti-poly, and Ti-poly images with a small FOV are taken with 3 rd set of AEC thresholds.  There are 7 different sets of AEC thresholds. (“0” means disable.) And, a dark image with the same FOV.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): an Active Region Observation Al-poly, and A-poly+Ti-poly images with a small FOV are taken with 1 st set of AEC thresholds.

Hinode Workshop / Hinode 専題研討会 /12/08-10 XRT Observation Table (XOB): an Active Region Observation The PROGram #09 continues with endless. The Subroutine #1 is called once in every 10 min*. The Subroutine #2 is called once in every 25 sec*.  * The duration becomes long, if exposure durations becomes long with AEC contols.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Timeline Synoptic AR Obs.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Timeline (cont.) Synoptic AR Obs. QS Obs.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Timeline (cont.) Synoptic QS Obs. AR Obs. Backup

Hinode Workshop / Hinode 専題研討会 /12/08-10 Data Rate The total data rate is estimated to 400kbps. XRT is typically allocated 15%. It corresponds ~ 600 k pixel / min, in the case of the DPCM compression. Kano et al. 2007, Solar Physics, in press.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Data Rate (cont.)

Hinode Workshop / Hinode 専題研討会 /12/08-10 In the Next Day … After the daily meeting, XRT-CO confirms that the XRT plan finally compiled by the chief planner (CP) has no error.

Hinode Workshop / Hinode 専題研討会 /12/08-10 Weekly Operations Once in a week, we usually do the followings.  Take a complete set of the dark images for near future the dark database.  Take a multi-filter full disk images.  Re-calibration of Focus position.