Increased Thermal Background for the post-NCS NICMOS

TIPS – June 19, 2003Megan Sosey

NICMOS

CycleCycle 11 Calibration Plan 11 Calibration Plan Parallel observations in NIC3:F222m,

NIC2: F222m & F237M were crafted to re-measure the thermal background for cycles 11 and beyond

-See proposals 9269 and 9702

Accounting for DQE increase, the average thermal background was predicted to be approximatly 20% higher than in Cycle 7

So, So, Where’sWhere’s the extra signal? the extra signal? NO correlation was found between the

variation in the thermal background and – telescope pointing – sun angle – prime instrument – time since SAA passage – or spacecraft orientation

The T-1-1 temperature sensor shows the detectors are stable under operation of the NCS and do not change by more than 0.1K on long time scales

Telescope Warm Season

Commanded Set-point change

T-1-1 Temperature Sensor vs. Time

9/10/2002 - 5/30/2003

Thermal Stability of the NICMOS Thermal Stability of the NICMOS Enclosure and Telescope AssemblyEnclosure and Telescope Assembly

NICMOS elements which affect the TB:re-imaging mirror (RM), FOM, PAM, filters, FDA(imaging mirrors), cold mask, bend mirrors, baffles, pupil

HST optics which affect the TB: primary mirror, secondary mirror, spiders,pads – these play significant roles in the TB because of their high temperatures (~290K)

Representation of Cold Mask Representation of Cold Mask MisalignmentMisalignment

See Robberto, Proc. SPIE v4013, p.386 and Krist, NICMOS-ISR-00-011 for more details on the cold mask alignment

Rough Optical Path Diagram for the Rough Optical Path Diagram for the NICMOS Fore-OpticsNICMOS Fore-Optics

Thermal stability of the HST Thermal stability of the HST optics and aft shroudoptics and aft shroud

The primary and secondary have remained thermally stable, introducing no extra thermal emission - however, the aft shroud has increased approximately 10K since Cycle 7

There are multiple thermistor sensors (thermally sensitive resistors) in the aft shroud which are used to monitor temperature

-TAFTBULK is a weighted average of the internal sensors located on the aft bulkhead

-TASINAFB is an effective sink measurement from all the internal sensors, including some of the ones from the TAFTBULK average

Thermal Environment of the HST Aft Thermal Environment of the HST Aft Shroud around NICMOS 2001-2002Shroud around NICMOS 2001-2002

Thermal Environment of the HST Aft Thermal Environment of the HST Aft Shroud around NICMOS 2001-2002Shroud around NICMOS 2001-2002

Aft Temperature Comparison of HST and Aft Temperature Comparison of HST and NICMOSNICMOS

naftbtmp

NIC3,

F222m

HST AFT

TASINAFB

TAFTBULK

C7 & C11 NICMOS Aft TempsC7 & C11 NICMOS Aft Temps

Key Descrip.

Avg. C7 Temp

Avg. C11 Temp Delta T

nfob2tmp Fore-optical brkt.

-5.82 C -0.48 C +5.34 C

ndosftmp Dewar Fore -7.27 C -1.21 C +6.06 C

ntrs3tmp Truss Aft 1.22 C 7.52 C +6.3 C

ndosatmp Dewar Aft -1.60 C 5.30 C +7.24 C

naftbtmp Aft NIC Encl. 8.5 C 17.5 C +9.0 C

taftbulk HST Aft Shroud

-17 C -7 C +10.0 C

NICMOSNICMOS Temperature Variations Temperature Variations

The NIC fore-optics swing in temperature in the same manner as the aft end, but with a smaller amplitude

Direct plot of thermal background vs fore-optics Direct plot of thermal background vs fore-optics temperaturetemperature

Does this explain the increase?Does this explain the increase?

The previous plot indicates that a 2K variation in temperature, translates to a 1.5DN change in the thermal background

An increase of 5K between Cycle 7 and Cycle 11 yields an additional 3DN of thermal background signal! - this makes up the difference between the predicted and observed thermal background

Simple blackbody comparison of HST and NICMOS Simple blackbody comparison of HST and NICMOS optical surfaces using NIC2 Optical Parameters optical surfaces using NIC2 Optical Parameters

Comparing to the NICMOS Thermal Comparing to the NICMOS Thermal Background Code EstimatesBackground Code Estimates

ConclusionsConclusionsThe overall temperature environment of NICMOS

and the operating temperature of the detectors has changed since cycle7 resulting in:

• Increase of ~17K in detector temperature• General temp. increase in the aft HST• Increased temperatures in the aft NICMOS• Increased thermal background in long

wavelength, or extra wide, camera 2 and camera 3 filters

• Thermal background exposures are still affective in removing the excess signal