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Geothermics
journal homepage: www.elsevier.com/locate/geothermics
Improved environmental monitoring of surface geothermal features through
comparisons of thermal infrared, satellite remote sensing and terrestrial
calorimetry
Anya Seward
a,
⁎
, Salman Ashraf
b
, Robert Reeves
a
, Chris Bromley
a
a
GNS Wairakei Research centre, Private bag 2000, Taupo, 3352, New Zealand
b
GNS Avalon, P.O. Box 30-368, Lower Hutt, 5040, New Zealand, New Zealand
ARTICLE INFO
Keywords:
Surface heat-loss
Thermal infrared
Remote sensing
Calorimetry
Satellite
Karapiti
New Zealand
ABSTRACT
Assessing changes in surface heat-loss at geothermally active areas provides insight into the geothermal re-
servoirs at depth. Surface temperatures and heat output of steam-heated ground can be inferred through pro-
cessing of thermal infrared images, as well as by direct measurements using terrestrial calorimetry. In February
2014, a high resolution aerial thermal infrared (TIR) survey and a terrestrial heat-loss survey (excluding fu-
marole discharge) were carried out over Karapiti (ca. 0.35 Km
2
in the Wairakei-Tauhara Geothermal System) in
the Taupo Volcanic Zone, New Zealand. Estimates of heat-loss are compared to those calculated from TIR data
collected by the Landsat-8 satellite of the area. This paper discusses the processing techniques for the datasets
and compares inferred surface heat losses. The aerial TIR and terrestrial measurements are in reasonable
agreement with calculated surface heat-loss values for Karapiti range from 41 MW (theoretical radiation heat
loss using aerial TIR) to 58 MW (total heat loss based on an empirical correlation with boiling-point depths).
Satellite images show a large variation between day-time and night-time TIR assessments. The assessment of
nocturnal (non-solar), radiation heat-loss is an order of magnitude lower than the total heat-loss determined
from the other techniques and approximately 1/3 of the inferred radiated component calculated from the aerial
TIR data. This is likely to be a consequence of diffuse, advecting-steam heat-loss, combined with an image
resolution issue: the pixel resolution of the satellite image (30 × 30 m) is much larger than the typical size of the
active geothermal surface manifestations (< 10 m
2
). Because the radiated heat-loss is a non-linear function of
land surface temperature, the in-pixel averaging under-estimates the radiated heat-loss. These and other pro-
blems currently restrict the usefulness of repeat low-resolution satellite imagery for monitoring of surface heat-
loss changes in steam-heated ground.
1. Introduction
The discharge of geothermal vapour from underground reservoirs
can result in areas of highly-heated and diffusely-steaming ground at
the surface. The amount of heat discharged can be indicative of the
relative size and recharge characteristics of the underlying geothermal
resource (Hochstein and Bromley, 2005). Accurate quantification and
monitoring of surface heat-loss in geothermal areas is difficult to
achieve, but is important for protecting the resource and its sur-
rounding environment. Such data is also important as an input for re-
servoir simulation modelling and for improved sustainable manage-
ment of geothermal fluid utilisation (e.g. Newson and O’Sullivan, 2004).
Improvements in monitoring tools and techniques are becoming in-
creasingly important in an environmentally conscientious society.
Advancements in capabilities, such as remote sensing, provide many
benefits to monitoring and assessing geothermal environments. They
reduce costs of land-based surveys, and meet increased safety con-
siderations for accessing geothermal areas. This paper compares heat-
loss estimations from terrestrial measurements, aerial thermal infrared
(TIR) images and satellite thermal imagery (TIRS) collected during
2014–2016, over the geothermal area at Karapiti, New Zealand. The
terms heat-loss and heat flux are used often throughout the text, with
heat flux referring to a measured surface heat output at a point
(W m
-2
), and heat-loss referring to the surface heat output over a to-
talled area (W).
The Karapiti thermal area (also known as “Craters of the Moon”) is
located within the Wairakei-Tauhara Geothermal System, in the Taupo
Volcanic Zone (TVZ), New Zealand (Fig. 1). It encompasses
https://doi.org/10.1016/j.geothermics.2018.01.007
Received 26 July 2017; Received in revised form 10 December 2017; Accepted 10 January 2018
⁎
Corresponding author.
E-mail address: a.seward@gns.cri.nz (A. Seward).
Geothermics 73 (2018) 60–73
Available online 03 February 2018
0375-6505/ © 2018 Elsevier Ltd. All rights reserved.
T