Top Banner
MARSCHALS: a new airborne millimetre-wave limb-sounder for the UTLS COST UTLS Workshop ESTEC, 11-13 March 2004 Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans, Brian Moyna, Matthew Oldfield, Dave Matheson Earth Observation and Atmospheric Science Division, SSTD
21

Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Jan 02, 2016

Download

Documents

MARSCHALS: a new airborne millimetre-wave limb-sounder for the UTLS COST UTLS Workshop ESTEC, 11-13 March 2004. Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans, Brian Moyna, Matthew Oldfield, Dave Matheson Earth Observation and Atmospheric Science Division, SSTD - PowerPoint PPT Presentation
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

MARSCHALS: a new airborne millimetre-wave

limb-sounder for the UTLS

COST UTLS WorkshopESTEC, 11-13 March 2004

Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans, Brian Moyna, Matthew Oldfield, Dave Matheson

Earth Observation and Atmospheric Science Division, SSTD Rutherford Appleton Laboratory

Page 2: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Introduction

• MARSCHALS

– Millimetre-wave Airborne Receiver for Spectroscopic CHaracterisation of Atmospheric Limb-Sounding

– a new airborne mm-wave limb sounder for the UTLS

– built under ESA contract by a consortium led by Rutherford Appleton Laboratory in the UK

• Contents

– Background, scientific rationale

– Instrument description

– Current status

– Future Plans

Page 3: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Marschals Objectives

• Demonstrate the capability of the mm-wave limb-sounding technique, to be employed by MASTER, to sound H2O, O3 and CO in the UT/LS region

– MASTER: proposed spaceborne limb sounder to measure thermal emission spectra at mm and sub-mm wavelengths

– mm-wave region: where extinction by aerosol and polar stratospheric clouds is negligible and extinction by cirrus clouds is low

• Participate in field campaigns in its own right (strat-trop exchange, radiative forcing, UT&LS chemistry)

Page 4: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

MARSCHALSon Geophysica

Page 5: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

The Marschals Instrument

• To simulate UTLS capabilities of MASTER as closely as possible, deployment on:– Geophysica near 20 km (primary carrier)

• Potential to retrieve horizontal and vertical structure in UTLS H2O, O3 and CO fields

– High-altitude balloon (secondary carrier) near 35 km• Capability for profile retrieval up to the mid-

stratosphere

Page 6: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Instrument Details

• MARSCHALS:– High efficiency antenna (22 cm) to make precise

elevation scans though the atmosphere– Heterodyne receiver concept– SSB receivers – 200 MHz spectral resolution (cf 50 MHz for MASTER)– Sideways viewing (cf rearwards for MASTER)

Page 7: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Instrument Details

• Bands:

– B: 294 - 305 GHz O3, pointing

– C: 316.5 – 325.5 GHz H2O

– D: 342.8 – 348.8 GHz CO– Modular design: more bands

can be added• Baseline scan sequence:

– -2 to 21 km in 1 km steps

Page 8: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

MASTER Bands

Page 9: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

OCM

• Optical Cloud Monitor:

– CCD array coupled to standard lens and broad-band filter (835-875nm)

– Records near-IR sunlight scattered in limb direction

• to identify cloud-free measurements for initial data analysis

• to indicate cloud conditions of each mm-wave measurement for analysis and interpretation, e.g.

– confirm mm-wave insensitivity to cloud

– relate mm-wave retrieved trace gas abundances to cloud

Page 10: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

SAGE-II Cloud Climatology

Page 11: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Cirrus Extinction vs Wavelength

Page 12: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Retrieval simulations - PrecisionBand B O3

MARSCHALS (aircraft)

MASTER

MARSCHALS (balloon)

% Error % Error

Alt

/ km

Alt

/ km

Band C H2O

% Error

Alt

/ km

Band D CO

Page 13: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Structural Test Model, May 2002

Page 14: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Structural Test Model, May 2002

Page 15: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Jan 2004

Page 16: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Current Status

• Instrument ~ 95% complete• Two RAL receivers, bands C and D, each with 12 GHz of

instantaneous bandwidth (@ 200MHz resolution)• Need to pass EMC test before flight• Characterisation of the full instrument is underway• L1 software ready

Page 17: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,
Page 18: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Deployment plans

• Funding for initial test flight and campaigns from EU APE-INFRA and ESA MALSAC

• Geophysica test flight March cancelled– Alternatives being investigated

• Rescheduled Geophysica flight (May/June earliest)• Jungfraujoch ?

• Scientific flights in future Geophysica campaigns– Alongside MIPAS-STR and SAFIRE-A

Page 19: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

Summary

• MARSCHALS– New mm-wave airborne limb sounder

– O3, H2O, CO and other trace gases in the UTLS

– First flight soon

• See poster: Tomographic limb-sounding of the Upper Troposphere and Lower Stratosphere– 2-D retrieval simulations for MASTER

Page 20: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,
Page 21: Victoria Jay, Brian Kerridge, Jolyon Reburn, Richard Siddans,

MARSCHALS L1 ATB ReviewBaseline Scan Sequence

– Scan -2km to 21km tangent height, integrating for 0.25s at each observation state.

– At each tangent height– 7 observations, 2 RF

switches: 50ms each– Total time per tangent

height: 2.2s– Total time for sequence:

52.8s (antenna motion during a cal.load view).

– In addition, limb scan– Starts hot/cold observation – Ends with cycle through all

bands at max. elevation (above horizontal).