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Development of a New Low-Cost Indoor Mapping System – System Design, System Calibration and First Results

Abstract

For mapping of building interiors various 2D and 3D indoor surveying systems are available today. These systems essentially differ from each other by price and accuracy as well as by the effort required for fieldwork and post-processing. The Laboratory for Photogrammetry & Laser Scanning of HafenCity University (HCU) Hamburg has developed, as part of an industrial project, a lowcost indoor mapping system, which enables systematic inventory mapping of interior facilities with low staffing requirements and reduced, measurable expenditure of time and effort. The modelling and evaluation of the recorded data take place later in the office. The indoor mapping system of HCU Hamburg consists of the following components: laser range finder, panorama head (pan-tilt-unit), single-board computer (Raspberry Pi) with digital camera and battery power supply. The camera is pre-calibrated in a photogrammetric test field under laboratory conditions. However, remaining systematic image errors are corrected simultaneously within the generation of the panorama image. Due to cost reasons the camera and laser range finder are not coaxially arranged on the panorama head. Therefore, eccentricity and alignment of the laser range finder against the camera must be determined in a system calibration. For the verification of the system accuracy and the system calibration, the laser points were determined from measurements with total stations. The differences to the reference were 4-5mm for individual coordinates.

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Development of a New Low-Cost Indoor Mapping System – System Design, System Calibration and First Results

Author: Kersten, Thomas,Stallmann, Dirk,Tschirschwitz, Felix
Publisher: Copernicus
DOI: 10.5194/isprs-archives-XLI-B5-55-2016
Source: https://repos.hcu-hamburg.de/bitstream/hcu/742/1/isprs-archives-XLI-B5-55-2016.pdf
DEVELOPMENT OF A NEW LOW-COST INDOOR MAPPING SYSTEM –
SYSTEM DESIGN, SYSTEM CALIBRATION AND FIRST RESULTS
T. P. Ke s en a*, D. S allmann a, F. Tschi schwi z a
a Ha enCi y Uni e si y Hambu g, Pho og amme y & Lase Scanning Lab, Übe seeallee 16, D-20457 Hambu g, Ge many -
(Thomas.Ke s en, Di k.S allmann, Felix.Tschi schwi z)@hcu-hambu g.de
Commission V, WG V/1
KEY WORDS: 3D, came a, calib a ion, modelling, spa se poin cloud, pano ama, econs uc ion
ABSTRACT:
Fo mapping o building in e io s a ious 2D and 3D indoo su eying sys ems a e a ailable oday. These sys ems essen ially di e
om each o he by p ice and accu acy as well as by he e o equi ed o ieldwo k and pos -p ocessing. The Labo a o y o
Pho og amme y & Lase Scanning o Ha enCi y Uni e si y (HCU) Hambu g has de eloped, as pa o an indus ial p ojec , a low-
cos indoo mapping sys em, which enables sys ema ic in en o y mapping o in e io acili ies wi h low s a ing equi emen s and
educed, measu able expendi u e o ime and e o . The modelling and e alua ion o he eco ded da a ake place la e in he o ice.
The indoo mapping sys em o HCU Hambu g consis s o he ollowing componen s: lase ange inde , pano ama head (pan- il -uni ),
single-boa d compu e (Raspbe y Pi) wi h digi al came a and ba e y powe supply. The came a is p e-calib a ed in a pho og amme ic
es ield unde labo a o y condi ions. Howe e , emaining sys ema ic image e o s a e co ec ed simul aneously wi hin he gene a ion
o he pano ama image. Due o cos easons he came a and lase ange inde a e no coaxially a anged on he pano ama head.
The e o e, eccen ici y and alignmen o he lase ange inde agains he came a mus be de e mined in a sys em calib a ion. Fo he
e i ica ion o he sys em accu acy and he sys em calib a ion, he lase poin s we e de e mined om measu emen s wi h o al s a ions.
The di e ences o he e e ence we e 4-5mm o indi idual coo dina es.
1. INTRODUCTION
Digi al building models ep esen he basis o planning,
cons uc ion and eno a ion as well as o he managemen o
buildings. In his con ex Building In o ma ion Modelling (BIM)
desc ibes a me hod o op imized h ee-dimensional planning,
execu ion o cons uc ion wo k and managemen o buildings by
app op ia e so wa e so ha all ele an building da a a e
digi ally eco ded, combined and in e connec ed. BIM applies
bo h in he building indus y o he building, planning and
execu ion o cons uc ion wo k (a chi ec u e, enginee ing,
building se ices), and in he acili y managemen sec o .
P ima ily, he a eas o buildings in he building and eal es a e
economy ep esen he basis o p ojec planning, cos ing and
income planning as well as o cons uc ion inancing. Since
building a eas a e also used o he appo ionmen o ope a ing
cos , incomple e, misleading o alse da a abou building a eas
can ha e ex ensi e, unwan ed consequences (Kalusche 2011).
Fo 90% o eal es a e in en o y a ea calcula ions a e no co ec
(P esseBox 2005, Wagne 2015). Thus he eal es a e indus y
uses inco ec da a abou building s ock in many cases, i.e.
eliable cu en da a is o en no a ailable a all.
In o de o measu e cu en a eas o p ope ies, di e en mode n
measu emen me hods such as e es ial lase scanning (Ke s en
e al. 2005, Ke s en & Linds aed 2012), digi al pho og amme y
(Ke s en e al. 2004) and achyme y a e a ailable, all o which
wo k sa is ac o ily o 3D eco ding o a chi ec u al objec s and
which a e es ablished in he ma ke . Howe e , hese p ocedu es
and sys ems equi e a ce ain le el o expe knowledge,
unde pinned by high acquisi ion and educa ion cos s. A lase -
pho og amme ic imaging sys em using pano ama pho og aphy
* Co esponding au ho
and lase anging in he opposi e axis o he came a was p esen ed
by Clauß (2011) and Clauß (2012). He ing (2012) showed in his
in es iga ions in o ins umen and model accu acy, ha his lase -
pho og amme ic imaging sys em is able o ensu e measu emen s
up o an accu acy o 2cm. Fangi (2007) p esen ed an app oach
whe e se e al sphe ical pano ama pho og aphs we e used o he
3D modelling o he in e io s o wo I alian chu ches.
Fu he mo e, so-called dep h senso s ( ime-o - ligh came as)
ha e al eady been used o he eco ding o in e io s (Zhu &
Donia 2013, Hen y e al. 2014). How seman ic in o ma ion can
be au oma ically ex ac ed om poin clouds de i ed om
pho og aphy o he in e io o BIM applica ions has been
desc ibed by Tamke e al. (2014) and K ispel e al. (2015).
The Labo a o y o Pho og amme y & Lase Scanning o he
Ha enCi y Uni e si y Hambu g is de eloping a low-cos imaging
sys em o in e io s in he con ex o a R&D coope a ion p ojec
o he cen al inno a ion p og amme (ZIM) o small and
medium-sized en e p ises (SMEs). Pa ne s in his p ojec a e he
Ins i u e o Compu e Science (Mul imedia In o ma ion
P ocessing) o he Ch is ian-Alb ech s Uni e si y Kiel, Ge many
and he company ETU So wa e GmbH om Cologne, Ge many.
The goal o his p ojec is o de elop new o signi ican ly
imp o e exis ing p oduc s, p ocesses and echnical se ices. In
he ollowing he sys em con igu a ion (chap e 2), he came a
and sys em calib a ion (chap e 3 and 4), he da a acquisi ion
(chap e 5) and he 3D modelling (chap e 6), including i s
esul s, will be desc ibed.
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
55
2. SYSTEM CONFIGURATION
The indoo mapping sys em o he HCU Hambu g is designed o
cap u e comple e 360° pano ama images o in e io spaces. The
o e all sys em consis s o a pano ama head wi h a came a, which
is i mly moun ed wi h a lase ange inde on a common
pla o m. The lase ange inde poin s in o he di ec ion o he
came a and measu es simul aneously a dis ance o a nonspeci ic
poin in he in e io o each aken pho o.
In o de o ge i s expe iences and acqui e es da a, a p o o ype
o he low-cos mapping sys em was buil a HCU Hambu g
using he ollowing componen s (Fig. 1):
1. Con ol compu e : Raspbe y Pi Model B
2. Digi al came a: Raspbe y Pi came a module
3. Lase ange inde : Bosch GLM 100 C P o essional
4. Powe supply: LogiLink powe bank
5. Pan- il uni : Man o o mul i-line pano ama head
6. Le elling de ice T ib ach wi h ubula le el
7. T ipod: Man o o ipod
The ad an ages o he selec ed ha dwa e a e:
(a) The cos s o he combina ion o Raspbe y Pi single-boa d
compu e and came a module a e e y a ou able wi h less han
60 EUR. (b) A la ge ange o accesso ies o a ious applica ions
al eady exis s o he Raspbe y Pi compu e . (c) Since he
compu e can be ope a ed wi h di e en Open-Sou ce 32-Bi
ope a ing sys ems, a e y ex ensi e o e ing o so wa e lib a ies
is a ailable. (d) The GPIO (gene al pu pose inpu /ou pu )
in e ace o he compu e can simply be used o he con ol o
senso s and displays. (e) The Bosch lase ange inde can be
comple ely con olled ia Blue oo h and he USB in e ace. ( )
The Man o o mul i-line pano ama head ul ils wo subs an ial
unc ions o he gene a ion o sphe ical pano amas:
1. The o a ion abou a second axis ( il ing axis), in o de o ake
pho og aphs wi h di e en e ical angles.
2. The mo emen o he came a a ound he en ance pupil o he
lens (nodal poin ).
Con ol so wa e wi h a simple use in e ace uns on he
Raspbe y Pi compu e , which enables acquisi ion o he images
and he dis ance measu emen s as well as he egis a ion o he
came a axes (ho izon al and e ical angles). The lase ange
inde is connec ed o he Raspbe y Pi compu e ia USB
in e ace. The Raspbe y Pi compu e is equipped wi h a WiFi
USB adap e , which se s up a local WLAN ne wo k, so ha he
sys em can be ope a ed by emo e connec ion om an ex e nal
pe sonal compu e , e.g. a lap op.
3. CAMERA CALIBRATION
To acqui e geome ically co ec in o ma ion om he pano amic
images, he digi al came a has been selec ed no only o cos
easons bu also by i s op ical cha ac e is ics such as scale,
dis o ion and s abili y. As a me hod o he objec i e alida ion
o hese c i e ia came a calib a ion in a 3D es ield was selec ed.
Fo he geome ical in es iga ions o he came a a he new
building loca ion o he HCU Hambu g a p o isional es ield
was es ablished (Fig. 2). The es ield has a size o 4.5m (wid h)
× 3.3m (heigh ) × 2.0m (dep h). The measu emen s o he con ol
poin s we e ca ied ou by a o al s a ion Leica TM30. Fo he
adjus men o he geode ic 3D ne wo k he p og am PANDA
om GEOTEC was used. The s anda d de ia ions o he adjus ed
con ol poin coo dina es we e 0.3mm (XY) in plane and 0.9mm
(Z) in dep h.
Figu e 2. Tempo a y 3D es ield o HCU Hambu g
Fo he came a calib a ion ou Raspbe y Pi came as (RPI 1, 2,
3, 4) wi h no mal angle lens (c = 3.6mm) and one came a (RPI 5)
wi h wide angle lens (c = 1.7mm) we e a ailable. The calib a ion
p ocedu e was epea ed wi h he di e en came as as indica ed in
Tab. 2.
The Raspbe y Pi Founda ion cu en ly o e s h ee di e en
came a modules. All came a modules ha e he same 5-Mega-
Pixel CMOS senso o he ype OmniVision OV5647 wi h 1.4
µm pixel spacing. The echnical speci ica ions o he Raspbe y
Pi came a a e summa ized in Tab. 1. The es ed came as a e
p obably no iden ically cons uc ed. They di e ou wa dly by
Figu e 1. Sys em componen s o he HCU 3D-IMAGER ( .l. . .): Raspbe y Pi compu e and came a, Bosch lase dis ance
measu ing ins umen , Man o o pano ama head, USB powe bank and he assembled HCU 3D-IMAGER sys em
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
56
he layou o he pla e and he insc ip ion o he chips. The cen al
componen , he OV5647 is p obably he same o all.
Un o una ely, no se ial numbe is used o clea iden i ica ion o
each came a module.
Came a OmniVision OV5647
Senso CMOS colou , 2592×1944 pix (5 MP)
Video 1080p wi h 30 ames/s, H.264 coding
Pixel size 1.4µm × 1.4µm
Senso size H×V 3.62mm × 2.72mm
Colou dep h 10 bi
In e ace CSI
Con ol Mul i-Media Abs ac ion Laye
Lens in eg a ed, ixed ocal leng h & ape u e
FoV H×V 54° × 41° (no mal angle)
Size H×W×D 25mm × 24mm × 9mm
Weigh 3 g
Table 1. Technical speci ica ions o he Raspbe y Pi came a
Fo came a calib a ion he bundle adjus men p og am Pic an
om Techne GmbH was used. The Pic an came a model
desc ibes he came a by h ee pa ame e s o in e io o ien a ion
(p inciple poin x0, y0 and came a cons an c) and by six
addi ional pa ame e s A1…A6 (sys ema ic image e o s),
whe eby A1 and A2 model he adial symme ic dis o ion o he
lens, A3 and A4 he a ini y and shea ing o he senso chip and
A5 and A6 he adial asymme ic and angen ial dis o ion o he
lens. The adjus ed nine pa ame e s o he in e io o ien a ion a e
summa ized in Table 2 a e calib a ion o i e di e en
Raspbe y Pi came as ( ou wi h no mal lens and one wi h wide
angle lens).
The e ec s o he addi ional pa ame e s on he image coo dina es
we e de e mined o he pa ame e g oups (A1, A2), (A3, A4)
and (A5, A6) sepa a ely and all oge he . These e ec s a e
ep esen ed in Fig. 3 wi h a 11 × 11 g id on he senso chip. The
g een g id shows he senso (chip size is 3.63mm × 2.72mm) and
he ed g id shows he e ec o he addi ional pa ame e s o
images coo dina es wi h 10 imes enla gemen .
Fo he calib a ed came as he ollowing esul s a e alid:
1. The e ec o he adial symme ic dis o ion (A1, A2) is
app oxima ely +20µm a he co ne s o he senso . The alues a e
simila o di e en came as modules (Fig. 4).
2. The e ec o a ini y and shea ing (A3, A4) is usually smalle
han 1µm.
3. The e ec o he adial asymme ic and angen ial dis o ion
(A5, A6) is usually smalle han 3µm.
The adial symme ic dis o ion has he la ges sys ema ic e ec
on he image coo dina es. All pa ame e s a e signi ican ly
de e mined in he bundle block adjus men . Fu he mo e, he
alues show li le a ia ion o he di e en came as.
Figu e 3. E ec o he addi ional pa ame e s (A1 … A6) on he
image coo dina es
The epea ed calib a ions show he ollowing esul s:
1. The came a cons an c a ied only sligh ly and seems o be
s able.
2. On he o he hand he posi ion o he p inciple poin shows
de ia ions up o 50 µm.
3. The adial symme ic dis o ion (A1, A2) a ied only sligh ly
and seems o be ela i e s able (Fig. 4).
4. The o he addi ional pa ame e s (a ini y and shea ing (A3,
A4) and adial asymme ic and angen ial dis o ion (A5,
A6)) demons a e no clea end. Howe e , hese las wo
pa ame e g oups only ha e a ela i ely small e ec on he
inal image coo dina es.
C M x0
[mm]
y0
[mm] c [mm] A1
[E-03]
A2
[E-03]
A3
[E-05]
A4
[E-05]
A5
[E-04]
A6
[E-05] Cal
RPI 1
1 -0.0304 0.0084 3.5864 5.67 -1.53 2.32 1.55 1.60 -2.95 15.04.14
2 0.0185 -0.0048 3.5851 5.74 -1.54 3.78 1.75 -1.98 2.22 26.06.14
3 -0.0230 -0.0001 3.5820 5.59 -1.50 2.90 2.68 1.89 -2.60 12.02.15
4 -0.0233 0.0003 3.5851 5.34 -1.43 48.30 1.09 1.85 -4.50 10.03.15
RPI 2
1 -0.0158 -0.0052 3.5892 5.37 -1.39 43.70 5.38 -1.80 -5.38 26.06.14
2 -0.0058 0.0346 3.5911 5.58 -1.44 46.00 -1.80 -3.64 -2.29 16.02.15
RPI 3
1 0.0096 -0.0371 3.6004 5.50 -1.45 46.60 -0.59 -1.39 -18.50 26.06.14
2 -0.0142 -0.0398 3.5999 5.40 -1.44 -0.48 0.85 0.99 20.00 12.02.15
3 -0.0154 -0.0409 3.6006 5.32 -1.38 44.50 0.49 1.07 15.70 10.03.15
RPI 4 1 0.0137 0.0042 3.5878 5.32 -1.40 46.40 4.82 1.42 -0.06 16.02.15
2 0.0128 0.0039 3.5880 5.27 -1.37 46.50 7.63 1.39 -2.97 18.02.15
RPI 5 1 0.0604 0.0042 1.7421 -77.00 3.66 104.00 17.80 3.17 -15.30 18.02.15
C…came as, M…measu emen s, x0/y0…p inciple poin , c…came a cons an , A1-A6…sys ema ic e o s, Cal… calib a ion da e
Table 2. In e io o ien a ion pa ame e se o di e en Raspbe y Pi came as
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
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Figu e 4. Radial symme ical dis o ion (A1, A2) o ou
di e en Raspbe y Pi came as ( op) and epe i ion o
calib a ions o a single came a (bo om)
The Raspbe y Pi came a has been compa ed wi h wo digi al
SLR came as (Nikon D700 and D90, bo h wi h 20mm lens) and
an indus ial came a IDS (wi h au o ocus) in a 3D es ield
calib a ion, in o de o ge in o ma ion abou he accu acy
po en ial o he low-cos came a. The esul s o he compa ison
a e summa ized in Table 3. The image measu ing accu acy o he
Raspbe y Pi came a wi h 0.2 pixels (1/5 pixel) is nea ly as good
as he SLR came as, while he empi ical accu acy (compa ison
o pho og amme ically de e mined poin s wi h he o al s a ion
e e ence) is wo se by he ac o 2-3, bu signi ican ly be e han
he indus ial came a.
4. SYSTEM CALIBRATION
The sys em calib a ion o he HCU 3D-IMAGER includes he
ollowing s eps: (a) he adap ion o he came a in he nodal poin
o he pano ama head and (b) he de e mina ion o he
eccen ici y and o ien a ion o he wo senso s (came a and lase
ange inde ). The en ance pupil o he came a lens mus lie
accu a ely in he nodal poin , since he ho izon al and e ical
o a ion o he came a mus be pe o med a ound he en ance
pupil o he lens. Du ing he came a o a ion a ound he en ance
pupil he lase ange inde o a es simul aneously on he
pano ama head. I is assumed ha he ela i e posi ion and
o a ion o he lase ange inde will no change wi h espec o
he came a. The e ical and ho izon al adjus men o he came a
is done sepa a ely ia alignmen on a close and a emo e poin .
The came a is shi ed un il he posi ion o he en ance pupil is
p ecisely ixed in he nodal poin using he alignmen pla es o
he pano ama head. An imp ecise alignmen leads o pa allaxes
a close ange while u ning he came a, which esul s in gaps in
he pano ama image. The ela i e posi ion o he lase ange
inde o he came a is de ined by a shi ec o (eccen ici y),
while he ela i e adjus men o he lase ange inde o he
came a is desc ibed by a di ec ion ec o . Thus he ela ion
be ween came a and lase ange inde is ep esen ed by a
coo dina e ans o ma ion wi h i e deg ees o eedom. The shi
ec o is measu ed wi h an accu acy o 1-2mm, while he
de e mina ion o he di ec ion ec o is pe o med wi h an
i e a i e me hod.
Fo he calib a ion and alida ion o he o e all sys em wo
pano ama images we e aken wi h h ee pho o se ies including 18
pho os each in he 3D es ield. The lase poin s we e measu ed
wi h a o al s a ion T imble S6 (measu emen 1) and/o wo
T imble 5603 DR200+ (measu emen 2a and b) as e e ence. The
p ecision (s anda d de ia ion) o he o al s a ions is 2” (=
0.6mgon) and/o 3” (= 1.0mgon) o an angle measu emen
(ho izon al and e ical) and 2mm + 2ppm o a dis ance
measu emen wi hou e lec o .
Came a I IP OP  xy [pix] SD PP [mm] C/Ch X [mm] Y [mm] Z [mm] max.  [mm]
D700_20 27 857 39 0.13 0.17 6/33 0.12 0.14 0.10 0.59
D90_20 36 1089 40 0.19 0.19 6/34 0.17 0.16 0.23 0.71
IDS XS 14 365 36 0.57 0.52 6/30 0.53 1.30 0.59 5.16
RPI 1 15 460 39 0.20 0.11 6/33 0.18 0.45 0.21 1.87
I….images, IP….image poin s, OP….objec poin s,

xy ….s anda d de ia ion o image coo dina es,
SD PP….s anda d de ia ion o con ol
p
oin s
,
C/Ch….con ol / check
p
oin s
,

XYZ….em
p
i ical accu ac
y
Table 3. S a is ics o he bundle block adjus men and empi ical accu acy o di e en came as in he 3D es ield in compa ison
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
58
The pola coo dina es o he lase poin s we e con e ed in o
Ca esian coo dina es, so ha bo h sys ems – lase poin s
measu ed by o al s a ion (sys em 1) and pano ama image
(sys em 2) – a e a ailable in he same coo dina e sys em. Fo
accu acy e alua ion he coo dina es o he lase poin s we e
ans o med dis o ion- ee by a spa ial simila i y ans o ma ion
(Helme ans o ma ion, 7-pa ame e ans o ma ion) in o he
pano ama coo dina e sys em (HCU 3D-IMAGER) (sys em 1 
sys em 2). Du ing an op imiza ion p ocess (a e Sansò 1973) he
se en ans o ma ion pa ame e s we e de e mined as ollows: a
spa ial shi ec o (3 pa ame e s), a scale ac o (1 pa ame e )
and a spa ial o a ion (3 pa ame e s). The ans o ma ion
pa ame e s we e de e mined using i e con ol poin s (#CP) in
each da ase . Fo he i e con ol poin s he RMS alues RMS
( ), RMS ( ) and RMS ( ) we e de e mined. The emaining
37 poin s we e used as checkpoin s (#ChP). The di e ences in
he checkpoin s we e de e mined as RMS alues (RMS (X),
RMS (Y), RMS (Z)). The esul s a e summa ized in Table 4.
The esidues o he con ol poin s a e be ween 2mm and 5mm
a e he adjus men . Howe e , he empi ical accu acy o he
checkpoin s is be ween 3mm o 11mm. The easons o hese
highe de ia ions a e accoun ed o by he measu emen s o he
lase poin and by he p ecision o he measu ing ins umen .
Since each lase poin shows as a ela i ely la ge i em in he
pho os and since he bo de o he lase poin is no well de ined,
he a ge ing o he lase poin cen e wi h he o al s a ion is no
always comple ely p ecise (see also Fig. 5). Fu he mo e, he
p ecision o he o al s a ion is limi ed due o he p ecision o he
( e lec o less) dis ance measu emen s o 2mm.
M Con ol Poin s RMS
[mm]
#
ChP
Check Poin s RMS
[mm]
X Y Z
1 3.5 2.7 4.1 37 3.9 2.9 2.9
2a 4.8 2.6 4.4 35 10.8 3.3 6.0
2b 2.3 1.4 1.8 37 6.3 2.6 6.6
M…Measu emen
,
ChP…Check Poin s
Table 4. Empi ical accu acy o lase poin s
o he HCU 3D-IMAGER using i e con ol poin s
5. 3D INDOOR DATA ACQUISITION
Fo in es iga ions in o 3D indoo mapping he calib a ed imaging
sys em HCU 3D-IMAGER has been used. The image acquisi ion
and he lase anging we e pe o med simul aneously, so ha he
ed lase poin is isible in each single image (Fig. 5). The
posi ioning o he sys em akes place in he cen e o small ooms
wi h su icien iew o all ele an co ne s o as an op imal
posi ioning con igu a ion, in o de o ealize op imal sigh
dis ances sho e han 15m. A e le elling he sys em, i is eady
o use. Fo he con olling o he sys em a lap op has been used,
o ope a e he con ol compu e Raspbe y Pi ia WLAN.
Figu e 6. Fi e image ows wi h 18 single images each o he gene a ion o one pano ama image
Figu e 5. Pa o a single pho o (le ) wi h snapped lase poin in he magni ied sec ions (cen e and igh )
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
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One single da a se consis s o a lase dis ance and a pho o (Fig.
5, igh ), which is sa ed on he Raspbe y Pi compu e oge he
wi h he o ien a ion pa ame e s o he aken pho o (ho izon al
angle in deg ees om ixed as e and e ical angles by eading
he scale). Depending upon desi ed imaging con igu a ion
(image o e lap) all ho izon al pho og aphs a e accomplished
wi h one e ical angula se ing. Fo a s anda d oom 18
ho izon al pho og aphs a e cu en ly used, which co esponds o
an o e lap ange o 51%. These 18 pho og aphs a e acqui ed a
di e en inclina ions, e.g. wi h he 5 inclina ion s ages +60°,
+30°, 0°, -30° and -50°, in o de o be able o compu e a ull-
sphe ical pano ama (Fig. 6). A lowe inclina ion is no necessa y,
since hese pho os will mainly show he pano ama head as well
as he ipod.
A e comple ion o he pho og aphy 360° sphe ical pano ama
images wi h a leas 12000 pixels o ho izon al esolu ion we e
gene a ed om he indi idually-acqui ed images. The ho izon al
and e ical angle, which a e de ined in a p ojec ile, we e used
as app oxima e alues o he de e mina ion o he exac
o a ions. These adjus ed o a ion angles a e he basis o he
calcula ion o he coo dina es o each lase poin in objec space.
The p oduc ion o a pano ama p oceeds in h ee s eps:
1. De e mina ion o gene al ie and special ie poin s on e ical
lines: Since he adjus men o he indi idual images canno
ake place wi h su icien accu acy, he pic u es a e linked by
homologous poin s in neighbou ing images.
2. Op imiza ion o he o ien a ion pa ame e s: Using hese ie
poin s he de e mina ion o image o ien a ion is in a
subsequen op imiza ion p ocess.
3. S i ching o he single images: Using he imp o ed image
o ien a ion he indi idual pho os a e s i ched o a pano ama
including b igh ness balancing.
Fo he s eps 1 and 2 he pano ama ools
(h p://pano ools.sou ce o ge.ne /) and o s ep 3 he CAU
S i che ( om he Ins i u e o Compu e Science o he
Ch is ian-Alb ech s Uni e si y Kiel) ha e been used.
Addi ionally, he CAU S i che compu es Ca esian 3D
coo dina es o each lase poin . Fo he ollowing 3D modelling
all cha ac e is ic pa ame e s a e w i en in o a p ojec ile and a e
he e o e consis en ly documen ed.
6. 3D MODELLING
Using only one indi idual pano ama image a scaled
econs uc ion o an indoo objec ( oom) is no possible.
Fu he mo e he 3D coo dina es o he lase poin s (see Fig. 7
small blue image), which ep esen he 3D oom as a e y spa se
poin cloud, do no allow a comple e econs uc ion o he objec .
In addi ion no all lase poin s a e p ojec ed on ele an plana
su aces. Only by combining he pano ama image and a leas one
Figu e 7. Gene a ed pano ama image and spa se poin cloud o he lase poin s (small blue image)
Figu e 8. 3D modelling – .l. . . de e mina ion o he g ound loo , de e mina ion o a wall, de e mina ion o he window opening
and example o a simple e-cons uc ed oom
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
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doi:10.5194/isp sa chi es-XLI-B5-55-2016
60
lase dis ance and by conside a ion o (geome ical) shape
condi ions can he oom be cons uc ed. The ollowing shape
condi ions suppo he modelling p ocess: De ini ion o spa ial
planes ( loo , ceiling and walls) o pe pendicula i y o wall
planes o loo plane o ceiling. Wi hin hese planes 2D su aces
( ec angles, iangles o ci cles) can be speci ied using he
pano ama image in he backg ound. The su aces can ep esen
walls, ceilings o openings (doo s, windows). The in e sec ion o
g ound loo , ceiling, and/o wall planes gene a es s aigh lines
di ec ly, which can be used as auxilia y lines o he cons uc ion
o he oom. The lase anging has essen ially he ask o
speci ying he scale o he econs uc ion.
On he basis o hese abo e men ioned model assump ions he
company ETU so wa e GmbH in Cologne has de eloped he 3D
modelling so wa e 3D BIS o manual modelling o in e io s.
Du ing he econs uc ion p ocess addi ional in o ma ion can be
speci ied, e.g. he labelling o objec pa s (g ound loo , ceiling,
wall, …), he ma e ial (s one, wood, PVC, …) and he s a us (OK,
ake down, epai , …). The so wa e adminis e s he indi idually-
acqui ed indoo da a and he associa ed me ada a, and
au oma ically compu es he solid and squa e measu e. Fo da a
exchange he cons uc ed 3D model can be expo ed in he
COLLADA o ma .
The econs uc ion o a oom wo ks wi h he 3D modelling
so wa e 3D BIS as ollows: On he condi ion ha he HCU 3D-
IMAGER has been se up pe pendicula ly on he g ound loo
and lase measu emen s o he g ound loo ook place, he
g ound le el can be cons uc ed. Wi hin he g ound plane he
loo plane can be cons uc ed nex by he de ini ion o 2D
su aces using he pano ama image in he backg ound (Fig. 8
igh , yellow su ace). On he condi ion ha he walls a e
pe pendicula o he g ound loo plane, he wall planes can be
cons uc ed a e wa ds (Fig. 8 cen e le , yellow su ace). Wi hin
he wall planes wall su aces and openings (windows and doo s)
Figu e 9. Gene a ed pano ama including depic ed lase poin s and modelled oom wi h slan ed walls
Figu e 10. Gene a ed pano ama and modelled oom which is unde cons uc ion
The In e na ional A chi es o he Pho og amme y, Remo e Sensing and Spa ial In o ma ion Sciences, Volume XLI-B5, 2016
XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
61
can be de e mined (Fig. 8 cen e igh , yellow su ace wi h
opening). A e all walls a e cons uc ed, he modelling o he
oom can be comple ed wi h he cons uc ion o he ceiling. The
inal 3D model can be expo ed o be u he p ocessed o
isualized in ano he 3D modelling so wa e (e.g. Ske chUp)
(Fig. 8 igh ). Fig. 9 shows he gene a ed pano ama pho o
including he isible lase poin s o ano he es objec and he
cons uc ed oom, while Fig. 10 ep esen s he gene a ed
pano ama image and he cons uc ed oom, which is in p ocess
o cons uc ion.
7. CONCLUSION AND OUTLOOK
The Labo a o y o Pho og amme y & Lase Scanning o he
HCU Hambu g de eloped a low-cos 3D imaging sys em o
in e io s, which does no cos mo e han 1000 EUR using he
cu en sys em s uc u e. The da a acquisi ion o in e io s using
he HCU 3D-IMAGER, which is equipped wi h a Raspbe y Pi
came a and a Bosch lase ange inde on a pano ama head,
cu en ly akes app ox. 12 minu es o a manual se ies o
indi idual pho os a ound 360° and lase dis ance measu emen s
o each image. The Raspbe y Pi came a used has small
dis o ion alues up o 20m, bu an uns able p inciple poin
(changes up o 50m). Ne e heless, he accu acy po en ial o he
Raspbe y Pi came a ob ained a e simul aneous came a
calib a ion does no qui e each he pe o mance o a digi al SLR
came a. A e sys em calib a ion an accu acy o app ox. 1cm o
single poin s can be expec ed o a s anda d in e io wi h
maximum dis ances o 10m. 20 ooms ha e al eady been
eco ded using his sys em and all could be econs uc ed om
he pano ama images and dis ance measu emen s using he
so wa e 3D-BIS.
In he u u e he 3D indoo mapping will wo k wi h a mo o ized
and compu e -con olled pano ama head, aking ewe pho os in
wo minu es pe s a ion. I is planned ha he wo k low om
pano ama p oduc ion o objec cons uc ion will be ully
suppo ed by au oma ic image p ocessing ope a ions. The
assump ion he e is ha he eco ded oom is mos ly o med om
simple wo dimensional elemen s, and ha he p edomina ing
pho o cha ac e is ics consis o a la ge ex en o ho izon al and
e ical s uc u es (Manha an Wo ld).
ACKNOWLEDGEMENTS
The suppo o he p ojec by ZIM ( he cen al inno a ion
p og amme o small and medium-sized en e p ises) – a
p og amme o he Fede al Minis y o Economic A ai s and
Ene gy – is g a e ul acknowledged.
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XXIII ISPRS Cong ess, 12–19 July 2016, P ague, Czech Republic
This con ibu ion has been pee - e iewed.
doi:10.5194/isp sa chi es-XLI-B5-55-2016
62